This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 9.04 00:09:30.11 +51:36:34.7
116.32775 -10.72356 galactic Cas Second-epoch detections are separated by 6.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:09:30.11 +51:36:34.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:30.11 +51:36:34.7: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:30.11 +51:36:34.7: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 09 30.11 +51 36 34.7 9.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,9.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 9.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 14.23 00:10:19.75 +53:23:15.6
116.74762 -8.98975 galactic Cas Second-epoch detections are separated by 7.6" and 8.3 pix
The object was found in VSX23" ZTF J001020.05+532252.3
Type: EW
# Max. Min./Amp. JD0 Period
17.436 g Y 0.693 g 2458469.66500 0.312260800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:19.75 +53:23:15.6: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:19.75 +53:23:15.6: 15.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 10 19.75 +53 23 15.6 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J001020.05+532252.3,2461251.8755,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J001020.05+532252.3 20260730.3755 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 14.27 00:03:21.89 +53:36:20.5
115.75403 -8.59474 galactic Cas Second-epoch detections are separated by 7.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:03:21.89 +53:36:20.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:21.89 +53:36:20.5: 15.74 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:21.89 +53:36:20.5: 15.98 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.74 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 03 21.89 +53 36 20.5 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 14.09 00:12:52.30 +55:53:13.4
117.50639 -6.57789 galactic Cas Second-epoch detections are separated by 5.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:12:52.30 +55:53:13.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:52.30 +55:53:13.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:52.30 +55:53:13.4: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 12 52.30 +55 53 13.4 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 14.05 00:11:29.57 +53:53:24.0
117.00044 -8.52108 galactic Cas Second-epoch detections are separated by 7.0" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:11:29.57 +53:53:24.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:29.57 +53:53:24.0: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:29.57 +53:53:24.0: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 11 29.57 +53 53 24.0 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 14.05CV 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 07 30.3755 2461251.8755 14.22 00:22:52.89 +53:18:18.1
118.61585 -9.32724 galactic Cas Second-epoch detections are separated by 4.8" and 7.8 pix
The object was found in VSX22" Gaia DR3 419109029081998720
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.500 G 13.550 G 0.096717000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:52.89 +53:18:18.1: 15.73 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:52.89 +53:18:18.1: 15.70 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.71 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 22 52.89 +53 18 18.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419109029081998720,2461251.8755,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419109029081998720 20260730.3755 14.22CV 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 07 30.3755 2461251.8755 13.95 00:20:03.11 +53:52:00.5
118.26044 -8.72002 galactic Cas Second-epoch detections are separated by 2.1" and 7.7 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 | 00:20:03.11 +53:52:00.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:03.11 +53:52:00.5: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:03.11 +53:52:00.5: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 20 03.11 +53 52 00.5 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 14.08 00:00:42.73 +53:45:27.4
115.39390 -8.37008 galactic Cas Second-epoch detections are separated by 6.9" and 8.1 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 | 00:00:42.73 +53:45:27.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:42.73 +53:45:27.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:42.73 +53:45:27.4: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 00 42.73 +53 45 27.4 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 14.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.91 00:10:58.19 +52:48:56.6
116.75129 -9.56971 galactic Cas Second-epoch detections are separated by 4.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J002.7450+52.8078 | 00:10:58.19 +52:48:56.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:58.19 +52:48:56.6: 15.32 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:58.19 +52:48:56.6: 15.95 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.32 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 10 58.19 +52 48 56.6 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.7450+52.8078,2461251.8755,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J002.7450+52.8078 20260730.3755 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.89 00:11:59.93 +52:33:28.9
116.86660 -9.84864 galactic Cas Second-epoch detections are separated by 3.1" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:11:59.93 +52:33:28.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:59.93 +52:33:28.9: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:59.93 +52:33:28.9: 15.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 11 59.93 +52 33 28.9 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.83 00:12:48.63 +53:58:07.0
117.20642 -8.47317 galactic Cas Second-epoch detections are separated by 5.2" and 8.0 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 | ATO J003.2091+53.9575 | 00:12:48.63 +53:58:07.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:48.63 +53:58:07.0: 15.51 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:48.63 +53:58:07.0: 15.16 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 12 48.63 +53 58 07.0 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.2091+53.9575,2461251.8755,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J003.2091+53.9575 20260730.3755 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.76 00:04:32.06 +52:54:22.9
115.79681 -9.31438 galactic Cas Second-epoch detections are separated by 0.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.1222+52.9025 | 00:04:32.06 +52:54:22.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:32.06 +52:54:22.9: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:32.06 +52:54:22.9: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 04 32.06 +52 54 22.9 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.1222+52.9025,2461251.8755,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.1222+52.9025 20260730.3755 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.72 00:12:09.80 +51:29:13.7
116.72368 -10.91057 galactic Cas Second-epoch detections are separated by 6.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:12:09.80 +51:29:13.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:09.80 +51:29:13.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:09.80 +51:29:13.7: 15.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 12 09.80 +51 29 13.7 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.60 00:28:05.45 +53:55:26.5
119.45793 -8.79016 galactic Cas Second-epoch detections are separated by 3.6" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:05.45 +53:55:26.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:28:05.45 +53:55:26.5: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:28:05.45 +53:55:26.5: 15.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 28 05.45 +53 55 26.5 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.66 23:39:40.19 +55:18:36.6
112.77552 -6.14004 galactic Cas Second-epoch detections are separated by 4.7" and 8.6 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 | 23:39:40.19 +55:18:36.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:40.19 +55:18:36.6: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:40.19 +55:18:36.6: 15.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 39 40.19 +55 18 36.6 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.61 00:27:40.62 +55:49:21.0
119.57474 -6.89429 galactic Cas Second-epoch detections are separated by 0.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:40.62 +55:49:21.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:27:40.62 +55:49:21.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:40.62 +55:49:21.0: 15.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 27 40.62 +55 49 21.0 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260730.3755 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.56 00:10:11.10 +50:58:17.2
116.32868 -11.37063 galactic Cas Second-epoch detections are separated by 8.0" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:10:11.10 +50:58:17.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:11.10 +50:58:17.2: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:11.10 +50:58:17.2: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 10 11.10 +50 58 17.2 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.61 23:52:27.39 +51:58:26.2
113.77520 -9.84609 galactic Cas Second-epoch detections are separated by 4.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:52:27.39 +51:58:26.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:27.39 +51:58:26.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:27.39 +51:58:26.2: 16.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 52 27.39 +51 58 26.2 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260730.3755 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.61 00:25:27.20 +52:39:45.1
118.93640 -10.00752 galactic Cas Second-epoch detections are separated by 2.3" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:27.20 +52:39:45.1 (user input) | T | P | (position from user input) J-Ks=0.891+/-0.067 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:27.20 +52:39:45.1: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:27.20 +52:39:45.1: 15.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 25 27.20 +52 39 45.1 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260730.3755 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.62 00:27:01.50 +51:15:17.1
119.03921 -11.43239 galactic Cas Second-epoch detections are separated by 2.1" and 8.1 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 | 00:27:01.50 +51:15:17.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:27:01.50 +51:15:17.1: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:01.50 +51:15:17.1: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 27 01.50 +51 15 17.1 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.59 00:03:44.40 +53:20:10.7
115.75861 -8.86982 galactic Cas Second-epoch detections are separated by 8.2" and 8.2 pix
The object was found in VSX 3" Gaia DR3 396202250502634240
Type: E
# Max. Min./Amp. JD0 Period
15.720 G 15.830 G 0.668830000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:44.40 +53:20:10.7: 15.68 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:44.40 +53:20:10.7: 15.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.68 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 03 44.40 +53 20 10.7 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 396202250502634240,2461251.8755,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 396202250502634240 20260730.3755 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.58 23:31:39.88 +56:54:31.0
112.16876 -4.28678 galactic Cas Second-epoch detections are separated by 3.4" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:31:39.88 +56:54:31.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:39.88 +56:54:31.0: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:39.88 +56:54:31.0: 15.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 31 39.88 +56 54 31.0 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.49 00:11:43.74 +54:49:49.8
117.18240 -7.59735 galactic Cas Second-epoch detections are separated by 2.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:11:43.74 +54:49:49.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:43.74 +54:49:49.8: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:43.74 +54:49:49.8: 15.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 11 43.74 +54 49 49.8 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.45 23:36:59.18 +56:58:33.6
112.88418 -4.43625 galactic Cas Second-epoch detections are separated by 1.5" and 8.6 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 | 23:36:59.18 +56:58:33.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:59.18 +56:58:33.6: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:59.18 +56:58:33.6: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 36 59.18 +56 58 33.6 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.28 00:20:54.23 +51:47:15.9
118.13347 -10.79929 galactic Cas Second-epoch detections are separated by 3.4" and 7.9 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 395087929829366016 | 00:20:50.08 +51:47:24.8 (Gaia DR3) | VAR (local) | 0.019146200000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:54.23 +51:47:15.9: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:54.23 +51:47:15.9: 15.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 20 54.23 +51 47 15.9 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395087929829366016,2461251.8755,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 395087929829366016 20260730.3755 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.44 23:22:09.42 +54:36:39.8
110.15443 -6.03064 galactic Cas Second-epoch detections are separated by 3.8" and 8.7 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 | 23:22:09.42 +54:36:39.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:09.42 +54:36:39.8: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:09.42 +54:36:39.8: 15.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 22 09.42 +54 36 39.8 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.38 00:24:22.96 +56:28:07.3
119.17966 -6.20582 galactic Cas Second-epoch detections are separated by 0.5" and 7.9 pix
The object was found in VSX20" Gaia DR3 421365433100482944
Type: ROT
# Max. Min./Amp. JD0 Period
15.010 G 15.070 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:22.96 +56:28:07.3: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:22.96 +56:28:07.3: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 24 22.96 +56 28 07.3 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421365433100482944,2461251.8755,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421365433100482944 20260730.3755 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.40 23:28:35.99 +50:40:52.8
109.77773 -10.06256 galactic And Second-epoch detections are separated by 8.2" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:35.99 +50:40:52.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:35.99 +50:40:52.8: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:35.99 +50:40:52.8: 15.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 28 35.99 +50 40 52.8 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.17 00:30:17.74 +55:33:35.7
119.92191 -7.18822 galactic Cas Second-epoch detections are separated by 6.2" and 7.6 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 | 00:30:17.74 +55:33:35.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:17.74 +55:33:35.7: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:17.74 +55:33:35.7: 15.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 30 17.74 +55 33 35.7 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.22 23:55:05.07 +54:12:31.8
114.67146 -7.75661 galactic Cas Second-epoch detections are separated by 6.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J358.7626+54.1925 | 23:55:01.85 +54:12:09.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:05.07 +54:12:31.8: 15.49 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:05.07 +54:12:31.8: 15.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.49 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 55 05.07 +54 12 31.8 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.7626+54.1925,2461251.8755,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.7626+54.1925 20260730.3755 13.22CV 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 07 30.3755 2461251.8755 13.21 00:21:11.81 +54:40:22.6
118.52639 -7.93992 galactic Cas Second-epoch detections are separated by 2.8" and 7.8 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 419828380261120256 | 00:21:08.10 +54:40:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:21:11.81 +54:40:22.6: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:21:11.81 +54:40:22.6: 15.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 21 11.81 +54 40 22.6 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419828380261120256,2461251.8755,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419828380261120256 20260730.3755 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.20 00:23:51.05 +55:31:01.4
119.00310 -7.14411 galactic Cas Second-epoch detections are separated by 5.0" and 7.8 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 421216582412687744 | 00:23:55.76 +55:31:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:51.05 +55:31:01.4: 15.72 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:51.05 +55:31:01.4: 15.37 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.47 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 23 51.05 +55 31 01.4 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421216582412687744,2461251.8755,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421216582412687744 20260730.3755 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.16 00:25:09.22 +53:39:27.9
118.99472 -9.01295 galactic Cas Second-epoch detections are separated by 3.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:09.22 +53:39:27.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:09.22 +53:39:27.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:09.22 +53:39:27.9: 15.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 25 09.22 +53 39 27.9 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.05 00:14:27.07 +56:43:29.1
117.84811 -5.78147 galactic Cas Second-epoch detections are separated by 2.5" and 7.9 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 | ATO J003.6271+56.7453 | 00:14:30.53 +56:44:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:27.07 +56:43:29.1: 14.77 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:27.07 +56:43:29.1: 14.98 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 14 27.07 +56 43 29.1 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.6271+56.7453,2461251.8755,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.6271+56.7453 20260730.3755 13.05CV 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 07 30.3755 2461251.8755 13.15 23:28:35.40 +57:13:31.0
111.86885 -3.85619 galactic Cas Second-epoch detections are separated by 5.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.1422+57.2370 | 23:28:35.40 +57:13:31.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:35.40 +57:13:31.0: 14.53 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:35.40 +57:13:31.0: 14.55 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 28 35.40 +57 13 31.0 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.1422+57.2370,2461251.8755,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.1422+57.2370 20260730.3755 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 12.97 23:58:38.59 +53:55:16.3
115.12510 -8.14838 galactic Cas Second-epoch detections are separated by 5.3" and 8.2 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 | 23:58:38.59 +53:55:16.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:38.59 +53:55:16.3: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:38.59 +53:55:16.3: 15.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 58 38.59 +53 55 16.3 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 12.94 00:30:27.03 +55:56:11.2
119.97500 -6.81476 galactic Cas Second-epoch detections are separated by 5.2" and 7.6 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 | ATO J007.6174+55.9537 | 00:30:29.60 +55:56:41.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:27.03 +55:56:11.2: 15.00 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:27.03 +55:56:11.2: 15.20 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 30 27.03 +55 56 11.2 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J007.6174+55.9537,2461251.8755,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J007.6174+55.9537 20260730.3755 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.04 23:55:26.74 +50:05:20.1
113.80979 -11.78849 galactic Cas Second-epoch detections are separated by 7.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:55:26.74 +50:05:20.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:26.74 +50:05:20.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:26.74 +50:05:20.1: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 55 26.74 +50 05 20.1 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 12.92 00:26:15.61 +55:46:37.8
119.37074 -6.92039 galactic Cas Second-epoch detections are separated by 5.2" and 7.7 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 | 00:26:15.61 +55:46:37.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:15.61 +55:46:37.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:15.61 +55:46:37.8: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 26 15.61 +55 46 37.8 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.03 00:06:17.54 +54:44:27.9
116.38773 -7.55602 galactic Cas Second-epoch detections are separated by 5.6" and 8.0 pix
The object was found in VSX 9" Gaia DR3 420397038232948096
Type: RS
# Max. Min./Amp. JD0 Period
17.000 G 17.070 G F
ATTENTION: measured mag 13.03 is 4.0 mag brighter than the VSX record maximum brightness 17.00 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:17.54 +54:44:27.9: 15.04 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:17.54 +54:44:27.9: 14.69 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 06 17.54 +54 44 27.9 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420397038232948096,2461251.8755,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420397038232948096 20260730.3755 13.03CV 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 07 30.3755 2461251.8755 13.02 23:10:22.38 +56:52:26.2
109.42014 -3.32284 galactic Cas Second-epoch detections are separated by 3.4" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J347.5927+56.8757 | 23:10:22.38 +56:52:26.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:22.38 +56:52:26.2: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:22.38 +56:52:26.2: 15.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 10 22.38 +56 52 26.2 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.5927+56.8757,2461251.8755,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.5927+56.8757 20260730.3755 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 12.93 00:25:47.94 +52:07:06.0
118.93350 -10.55426 galactic Cas Second-epoch detections are separated by 4.2" and 8.3 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 | 00:25:47.94 +52:07:06.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:47.94 +52:07:06.0: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:47.94 +52:07:06.0: 15.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 25 47.94 +52 07 06.0 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 12.79 23:22:08.26 +54:51:02.0
110.23363 -5.80445 galactic Cas Second-epoch detections are separated by 8.0" and 8.6 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 | ATO J350.5294+54.8578 | 23:22:08.26 +54:51:02.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:08.26 +54:51:02.0: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:08.26 +54:51:02.0: 15.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 22 08.26 +54 51 02.0 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.5294+54.8578,2461251.8755,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.5294+54.8578 20260730.3755 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 11.93 00:13:48.86 +52:27:47.7
117.12925 -9.98409 galactic Cas Second-epoch detections are separated by 5.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:13:48.86 +52:27:47.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:48.86 +52:27:47.7: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:48.86 +52:27:47.7: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 13 48.86 +52 27 47.7 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 11.79 00:14:00.15 +51:35:37.6
117.02794 -10.84832 galactic Cas Second-epoch detections are separated by 2.4" and 8.0 pix
The object was found in VSX 9" Gaia DR3 395014743582908672
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.800 G 13.840 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:00.15 +51:35:37.6: 14.12 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:00.15 +51:35:37.6: 14.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 14 00.15 +51 35 37.6 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395014743582908672,2461251.8755,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 395014743582908672 20260730.3755 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 11.47 00:15:10.33 +53:13:09.0
117.44611 -9.26586 galactic Cas Second-epoch detections are separated by 3.3" and 7.9 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 | ATO J003.7966+53.2276 | 00:15:10.33 +53:13:09.0 (user input) | STOCH (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:10.33 +53:13:09.0: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:10.33 +53:13:09.0: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 15 10.33 +53 13 09.0 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.7966+53.2276,2461251.8755,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.7966+53.2276 20260730.3755 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 12.99 00:23:20.52 +55:49:18.3
118.96461 -6.83342 galactic Cas Second-epoch detections are separated by 6.1" and 7.6 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 | ATO J005.8518+55.8256 | 00:23:20.52 +55:49:18.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:20.52 +55:49:18.3: 14.82 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:20.52 +55:49:18.3: 14.48 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 23 20.52 +55 49 18.3 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J005.8518+55.8256,2461251.8755,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J005.8518+55.8256 20260730.3755 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 12.99 23:58:01.28 +50:30:16.1
114.31109 -11.47101 galactic Cas Second-epoch detections are separated by 1.7" and 8.6 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 | 23:58:01.28 +50:30:16.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:01.28 +50:30:16.1: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:01.28 +50:30:16.1: 15.21 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 58 01.28 +50 30 16.1 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.10 00:20:02.57 +50:09:43.6
117.79304 -12.39612 galactic Cas Second-epoch detections are separated by 6.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J005.0247+50.1555 | 00:20:02.57 +50:09:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:02.57 +50:09:43.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:02.57 +50:09:43.6: 15.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 20 02.57 +50 09 43.6 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J005.0247+50.1555,2461251.8755,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J005.0247+50.1555 20260730.3755 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.15 23:57:59.98 +50:31:00.1
114.31027 -11.45834 galactic Cas Second-epoch detections are separated by 2.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:57:59.98 +50:31:00.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:59.98 +50:31:00.1: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:59.98 +50:31:00.1: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 57 59.98 +50 31 00.1 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.20 00:24:48.07 +53:02:40.7
118.87715 -9.61727 galactic Cas Second-epoch detections are separated by 2.0" and 7.6 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 | 00:24:48.07 +53:02:40.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:48.07 +53:02:40.7: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:48.07 +53:02:40.7: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 24 48.07 +53 02 40.7 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.21 23:56:30.03 +53:45:20.0
114.77780 -8.24416 galactic Cas Second-epoch detections are separated by 7.3" and 8.2 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 | 23:56:30.03 +53:45:20.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:30.03 +53:45:20.0: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:30.03 +53:45:20.0: 15.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 56 30.03 +53 45 20.0 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.42 23:33:45.39 +52:44:43.4
111.19406 -8.34693 galactic Cas Second-epoch detections are separated by 8.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:33:45.39 +52:44:43.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:45.39 +52:44:43.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:45.39 +52:44:43.4: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 33 45.39 +52 44 43.4 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.30 00:12:54.65 +50:00:36.7
116.61149 -12.38816 galactic Cas Second-epoch detections are separated by 3.2" and 8.3 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 | 00:12:54.65 +50:00:36.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:54.65 +50:00:36.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:54.65 +50:00:36.7: 15.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 12 54.65 +50 00 36.7 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.37 23:55:17.18 +50:18:36.8
113.83414 -11.56700 galactic Cas Second-epoch detections are separated by 6.1" and 8.4 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 | 23:55:17.18 +50:18:36.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:17.18 +50:18:36.8: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:17.18 +50:18:36.8: 15.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 55 17.18 +50 18 36.8 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.46 23:59:00.94 +53:17:41.6
115.05014 -8.77273 galactic Cas Second-epoch detections are separated by 4.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:59:00.94 +53:17:41.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:59:00.94 +53:17:41.6: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:00.94 +53:17:41.6: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 59 00.94 +53 17 41.6 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260730.3755 13.46CV 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 07 30.3755 2461251.8755 13.40 00:12:00.96 +53:37:01.0
117.03488 -8.80282 galactic Cas Second-epoch detections are separated by 7.1" and 7.9 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 | ATO J003.0116+53.6176 | 00:12:00.96 +53:37:01.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:00.96 +53:37:01.0: 14.28 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:00.96 +53:37:01.0: 14.53 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 12 00.96 +53 37 01.0 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.0116+53.6176,2461251.8755,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.0116+53.6176 20260730.3755 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.71 23:12:16.25 +55:19:37.7
109.08038 -4.85508 galactic Cas Second-epoch detections are separated by 6.9" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996710440285756288 | 23:12:17.96 +55:18:55.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:16.25 +55:19:37.7: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:16.25 +55:19:37.7: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 12 16.25 +55 19 37.7 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996710440285756288,2461251.8755,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996710440285756288 20260730.3755 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.39 00:07:55.48 +53:41:36.5
116.44227 -8.62910 galactic Cas Second-epoch detections are separated by 2.1" and 8.1 pix
The object was found in VSX21" Gaia DR3 420056189628253696
Type: ROT
# Max. Min./Amp. JD0 Period
16.210 G 16.250 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:55.48 +53:41:36.5: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:55.48 +53:41:36.5: 15.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 07 55.48 +53 41 36.5 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420056189628253696,2461251.8755,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420056189628253696 20260730.3755 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.45 00:22:41.40 +56:26:52.0
118.94357 -6.20119 galactic Cas Second-epoch detections are separated by 2.6" and 7.7 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 | 00:22:41.40 +56:26:52.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:41.40 +56:26:52.0: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:41.40 +56:26:52.0: 15.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 22 41.40 +56 26 52.0 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.49 23:28:24.80 +57:49:21.2
112.03523 -3.28197 galactic Cas Second-epoch detections are separated by 6.7" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:24.80 +57:49:21.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:24.80 +57:49:21.2: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:24.80 +57:49:21.2: 15.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 28 24.80 +57 49 21.2 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.46 23:19:50.25 +55:37:38.0
110.19251 -4.96242 galactic Cas Second-epoch detections are separated by 5.8" and 8.6 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 | 23:19:50.25 +55:37:38.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:50.25 +55:37:38.0: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:50.25 +55:37:38.0: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 19 50.25 +55 37 38.0 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260730.3755 13.46CV 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 07 30.3755 2461251.8755 13.51 00:13:54.18 +55:16:27.8
117.56014 -7.20539 galactic Cas Second-epoch detections are separated by 8.8" and 7.7 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 | 00:13:54.18 +55:16:27.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:54.18 +55:16:27.8: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:54.18 +55:16:27.8: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 13 54.18 +55 16 27.8 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.54 00:19:38.02 +50:48:48.7
117.81033 -11.74168 galactic Cas Second-epoch detections are separated by 4.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:38.02 +50:48:48.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:38.02 +50:48:48.7: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:38.02 +50:48:48.7: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 19 38.02 +50 48 48.7 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.69 00:27:12.05 +54:06:10.9
119.34314 -8.59975 galactic Cas Second-epoch detections are separated by 6.1" and 7.6 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 419566769506900736 | 00:27:07.88 +54:06:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:27:12.05 +54:06:10.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:12.05 +54:06:10.9: 15.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 27 12.05 +54 06 10.9 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419566769506900736,2461251.8755,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 419566769506900736 20260730.3755 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.65 23:50:26.63 +54:13:52.6
114.01011 -7.58051 galactic Cas Second-epoch detections are separated by 7.5" and 8.2 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 | 23:50:26.63 +54:13:52.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:26.63 +54:13:52.6: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:26.63 +54:13:52.6: 15.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 50 26.63 +54 13 52.6 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.72 00:24:22.17 +53:19:57.7
118.84276 -9.32400 galactic Cas Second-epoch detections are separated by 7.2" and 8.0 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 | ATO J006.0983+53.3364 | 00:24:22.17 +53:19:57.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:22.17 +53:19:57.7: 14.52 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:22.17 +53:19:57.7: 14.92 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 24 22.17 +53 19 57.7 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J006.0983+53.3364,2461251.8755,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.0983+53.3364 20260730.3755 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.86 23:21:34.07 +55:55:46.4
110.52624 -4.76239 galactic Cas Second-epoch detections are separated by 2.8" and 8.7 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 | ATO J350.3845+55.9274 | 23:21:34.07 +55:55:46.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:34.07 +55:55:46.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:34.07 +55:55:46.4: 15.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 21 34.07 +55 55 46.4 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.3845+55.9274,2461251.8755,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.3845+55.9274 20260730.3755 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.87 00:12:48.56 +55:50:46.5
117.49152 -6.61692 galactic Cas Second-epoch detections are separated by 8.3" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:12:48.56 +55:50:46.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:48.56 +55:50:46.5: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:48.56 +55:50:46.5: 15.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 12 48.56 +55 50 46.5 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260730.3755 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 14.06 23:51:05.94 +53:56:13.3
114.03457 -7.88910 galactic Cas Second-epoch detections are separated by 7.3" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:51:05.94 +53:56:13.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:05.94 +53:56:13.3: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:51:05.94 +53:56:13.3: 15.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 51 05.94 +53 56 13.3 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 14.26 00:02:01.52 +52:37:15.8
115.36452 -9.52316 galactic Cas Second-epoch detections are separated by 8.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:02:01.52 +52:37:15.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:01.52 +52:37:15.8: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:01.52 +52:37:15.8: 15.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 02 01.52 +52 37 15.8 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 12.30 23:20:43.39 +54:46:57.7
110.01784 -5.79845 galactic Cas Second-epoch detections are separated by 5.1" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:20:43.39 +54:46:57.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:43.39 +54:46:57.7: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:43.39 +54:46:57.7: 15.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 20 43.39 +54 46 57.7 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461251.8755,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260730.3755 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 12.02 23:21:42.35 +50:06:37.3
108.53226 -10.23581 galactic And Second-epoch detections are separated by 2.5" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.4335+50.1053 | 23:21:42.35 +50:06:37.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:42.35 +50:06:37.3: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:42.35 +50:06:37.3: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 23 21 42.35 +50 06 37.3 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.4335+50.1053,2461251.8755,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.4335+50.1053 20260730.3755 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3755 2461251.8755 13.44 00:04:11.85 +54:17:11.6
116.00342 -7.94847 galactic Cas Second-epoch detections are separated by 6.9" and 8.1 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 J001.0596+54.2914 | 00:04:11.85 +54:17:11.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:11.85 +54:17:11.6: 15.43 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:11.85 +54:17:11.6: 15.60 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.51 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 30.3755* 00 04 11.85 +54 17 11.6 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.0596+54.2914,2461251.8755,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.0596+54.2914 20260730.3755 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461251.87587703 30.07.2026 09:01:05.775 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 5 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): 21448
Objects passed selection criteria: 21393
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 17353.8
Average stars matched: 16449.5 (94.7893 %)
Memory usage VmPeak: 248488 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 30 04:24:14 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: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461251.87587703 30.07.2026 09:01:05.775 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 253
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: 82 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): 160731
Objects passed selection criteria: 160376
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 140140
Average stars matched: 133661 (95.3762 %)
Memory usage VmPeak: 632520 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 30 04:28:17 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.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: 2461251.87521264
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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.059 +54:00:13.58 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Image size: 926.7'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:58.292 +54:00:51.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.059 +54:00:13.58
Second-epoch image center 23:59:58.292 +54:00:51.92
Angular distance between the image centers 0.0115 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Image size: 926.7'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:55.971 +54:01:36.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.059 +54:00:13.58
Second-epoch image center 23:59:55.971 +54:01:36.25
Angular distance between the image centers 0.0250 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:58.292 +54:00:51.92
Second-epoch second image center 23:59:55.971 +54:01:36.25
Angular distance between the image centers 0.01356 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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.gNGTvUEsrg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.4Qc1KvbMf7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits &> /tmp/tmp.W1IoDzipis
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits &> /tmp/tmp.CyAoRDge9B
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0161 to 14.8837 deg, Dec +48.1259 to +59.2680 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 345.0161 to 14.8837 deg, Dec 48.1259 to 59.2680 deg
Loaded 25395 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): 16157 out of 17527 total matches.
Matched with Tycho-2 17527 out of 28951 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.643500
a=0.000000 b=1.000000 c=22.643500
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.97
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.97
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0161 to 14.8837 deg, Dec +48.1259 to +59.2680 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 345.0161 to 14.8837 deg, Dec 48.1259 to 59.2680 deg
Loaded 25395 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): 16157 out of 17527 total matches.
Matched with Tycho-2 17527 out of 28951 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=6.3)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 32399 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0247 to 14.8783 deg, Dec +48.1255 to +59.2627 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 345.0247 to 14.8783 deg, Dec 48.1255 to 59.2627 deg
Loaded 25378 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): 15455 out of 16923 total matches.
Matched with Tycho-2 16923 out of 32399 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.3 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Limiting magnitude estimates:
15.0 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
15.1 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
14.3 mag. fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
14.3 mag. fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gNGTvUEsrg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2748, bad_region=6855, passed=28951
Got 28951 stars (including 19826 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 28951 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
RA wraps around 0/360 boundary: field RA 345.0161 through 0 to 14.8837, gap 14.8837 to 345.0161
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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 4917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 23647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0140 through 0 to 14.8842, gap 14.8842 to 345.0140
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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 23647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 23647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4917 stars left (next iteration limit 5408)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=4917 sigma_overall_arcsec=0.503 sigma_q1_arcsec=0.457 sigma_q2_arcsec=0.471 sigma_q3_arcsec=0.531 sigma_q4_arcsec=0.505 n_q1=1481 n_q2=914 n_q3=1523 n_q4=999 worst_quadrant_to_overall_ratio=1.054
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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.4Qc1KvbMf7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3204, bad_region=7312, passed=32399
Got 32399 stars (including 22421 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 32399 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
RA wraps around 0/360 boundary: field RA 345.0247 through 0 to 14.8783, gap 14.8783 to 345.0247
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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 26793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0147 through 0 to 14.8781, gap 14.8781 to 345.0147
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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 26793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 26793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4912 stars left (next iteration limit 5401)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=4912 sigma_overall_arcsec=0.512 sigma_q1_arcsec=0.460 sigma_q2_arcsec=0.506 sigma_q3_arcsec=0.524 sigma_q4_arcsec=0.538 n_q1=1489 n_q2=908 n_q3=1517 n_q4=998 worst_quadrant_to_overall_ratio=1.050
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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.W1IoDzipis (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1278, bad_region=3324, passed=14660
Got 14660 stars (including 10294 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat
util/solve_plate_with_UCAC5 got 14660 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.1050 through 0 to 14.8816, gap 14.8816 to 345.1050
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3494 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2143 matched stars entering correct_measured_positions(), 2371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2001 matched stars entering correct_measured_positions(), 11854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.90"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.1066 through 0 to 14.8997, gap 14.8997 to 345.1066
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3578 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2415 matched stars entering correct_measured_positions(), 11855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.11"
Accuracy estimation diagnostic: 2327 matched stars entering correct_measured_positions(), 11875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.04"
Excluding outliers - 2327 stars left (next iteration limit 2201)
SIP_REFIT: SIP order 2 trial: matched=2327 robust_rms=26.271 arcsec worst_quadrant_rms=28.201 arcsec
SIP_REFIT: SIP order 3 trial: matched=2327 robust_rms=25.529 arcsec worst_quadrant_rms=28.558 arcsec
SIP_REFIT: SIP order 5 trial: matched=2327 robust_rms=23.170 arcsec worst_quadrant_rms=28.128 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2327 robust_rms_before=31.677 arcsec robust_rms_before_corrected=19.376 arcsec robust_rms_after=26.271 arcsec worst_quadrant_rms_before=24.088 worst_quadrant_rms_after=28.201
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.088 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits N_match=2327 sigma_overall_arcsec=13.896 sigma_q1_arcsec=28.974 sigma_q2_arcsec=29.229 sigma_q3_arcsec=7.727 sigma_q4_arcsec=5.999 n_q1=514 n_q2=262 n_q3=901 n_q4=650 worst_quadrant_to_overall_ratio=2.103
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.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.CyAoRDge9B (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1254, bad_region=3331, passed=14612
Got 14612 stars (including 10253 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat
util/solve_plate_with_UCAC5 got 14612 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.1053 through 0 to 14.8809, gap 14.8809 to 345.1053
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3493 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2154 matched stars entering correct_measured_positions(), 2376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2024 matched stars entering correct_measured_positions(), 11767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.96"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.1069 through 0 to 14.8989, gap 14.8989 to 345.1069
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3580 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2403 matched stars entering correct_measured_positions(), 11768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.18"
Accuracy estimation diagnostic: 2322 matched stars entering correct_measured_positions(), 11841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.05"
Excluding outliers - 2322 stars left (next iteration limit 2226)
SIP_REFIT: SIP order 2 trial: matched=2322 robust_rms=26.384 arcsec worst_quadrant_rms=28.915 arcsec
SIP_REFIT: SIP order 3 trial: matched=2322 robust_rms=25.527 arcsec worst_quadrant_rms=29.048 arcsec
SIP_REFIT: SIP order 5 trial: matched=2322 robust_rms=23.296 arcsec worst_quadrant_rms=29.058 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2322 robust_rms_before=31.894 arcsec robust_rms_before_corrected=19.259 arcsec robust_rms_after=26.384 arcsec worst_quadrant_rms_before=24.414 worst_quadrant_rms_after=28.915
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.414 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits N_match=2322 sigma_overall_arcsec=13.571 sigma_q1_arcsec=28.175 sigma_q2_arcsec=27.162 sigma_q3_arcsec=7.081 sigma_q4_arcsec=5.898 n_q1=510 n_q2=269 n_q3=902 n_q4=641 worst_quadrant_to_overall_ratio=2.076
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.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=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits sigma_overall=0.503 worst_q_ratio=1.054
ref2=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits sigma_overall=0.512 worst_q_ratio=1.050
new1=fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits sigma_overall=13.896 worst_q_ratio=2.103
new2=fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits sigma_overall=13.571 worst_q_ratio=2.076
reference average sigma_overall=0.5075 worst_q_ratio=1.052
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits) flagged: sigma=13.896 (ref avg 0.5075), ratio=2.103 (ref avg 1.052), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/lib/make_outxyls_for_astrometric_calibration found 14144 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2457762.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2457762.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 23.4524 (1.5319e+10), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.99,54.0128), pixel scale 5.93115 arcsec/pix.
Hit/miss: Hit/miss: -+--+--------++-+---+-----+(best)-----+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2457762.solved to indicate this.
Field: out2457762.xyls
Field center: (RA,Dec) = (359.991484, 54.013608) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.956, +54:00:48.988).
Field size: 15.6058 x 10.4321 degrees
Field rotation angle: up is 4.4499 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits' -> 'fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 30 04:26 fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
-rw-r--r-- 1 apache apache 8.5K Jul 30 04:26 out2457762.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits (fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out2457762.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2457762.axy"...
Only searching for solutions within 15.445 degrees of RA,Dec (359.993,54.0144)
log-odds ratio 23.4524 (1.5319e+10), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.99,54.0128), pixel scale 5.93115 arcsec/pix.
Hit/miss: Hit/miss: -+--+--------++-+---+-----+(best)-----+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2457762.solved to indicate this.
Field: out2457762.xyls
Field center: (RA,Dec) = (359.991484, 54.013608) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.956, +54:00:48.988).
Field size: 15.6058 x 10.4321 degrees
Field rotation angle: up is 4.4499 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 30 04:26 fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
-rw-r--r-- 1 apache apache 8.5K Jul 30 04:26 out2457762.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat from image00003.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Image size: 926.7'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:58.292 +54:00:51.92 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 14660 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/correct_sextractor_wcs_catalog_usingxy2sky2459062.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1278, bad_region=3324, passed=14660
Got 14660 stars (including 10294 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat
util/solve_plate_with_UCAC5 got 14660 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.1050 through 0 to 14.8816, gap 14.8816 to 345.1050
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3494 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2143 matched stars entering correct_measured_positions(), 2371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2001 matched stars entering correct_measured_positions(), 11854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.90"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.1066 through 0 to 14.8997, gap 14.8997 to 345.1066
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3578 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2415 matched stars entering correct_measured_positions(), 11855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.11"
Accuracy estimation diagnostic: 2327 matched stars entering correct_measured_positions(), 11875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.04"
Excluding outliers - 2327 stars left (next iteration limit 2201)
SIP_REFIT: SIP order 2 trial: matched=2327 robust_rms=26.271 arcsec worst_quadrant_rms=28.201 arcsec
SIP_REFIT: SIP order 3 trial: matched=2327 robust_rms=25.529 arcsec worst_quadrant_rms=28.558 arcsec
SIP_REFIT: SIP order 5 trial: matched=2327 robust_rms=23.170 arcsec worst_quadrant_rms=28.128 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2327 robust_rms_before=31.677 arcsec robust_rms_before_corrected=19.376 arcsec robust_rms_after=26.271 arcsec worst_quadrant_rms_before=24.088 worst_quadrant_rms_after=28.201
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.088 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits N_match=2327 sigma_overall_arcsec=13.896 sigma_q1_arcsec=28.974 sigma_q2_arcsec=29.229 sigma_q3_arcsec=7.727 sigma_q4_arcsec=5.999 n_q1=514 n_q2=262 n_q3=901 n_q4=650 worst_quadrant_to_overall_ratio=2.103
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits): sigma 13.896->13.896, ratio 2.103->2.103; reverting to order 3
WCS_QUALITY_RETRY: 2nd new image (fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits) flagged: sigma=13.571 (ref avg 0.5075), ratio=2.076 (ref avg 1.052), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/lib/make_outxyls_for_astrometric_calibration found 14118 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2459697.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2459697.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 22.9458 (9.23068e+09), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.98,54.0251), pixel scale 5.93124 arcsec/pix.
Hit/miss: Hit/miss: -+--+--------++-+---+-----+(best)-----+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2459697.solved to indicate this.
Field: out2459697.xyls
Field center: (RA,Dec) = (359.981813, 54.025922) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:55.635, +54:01:33.320).
Field size: 15.6061 x 10.4325 degrees
Field rotation angle: up is 4.46177 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits' -> 'fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 30 04:26 fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
-rw-r--r-- 1 apache apache 8.5K Jul 30 04:26 out2459697.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits (fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out2459697.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2459697.axy"...
Only searching for solutions within 15.445 degrees of RA,Dec (359.983,54.0267)
log-odds ratio 22.9458 (9.23068e+09), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.98,54.0251), pixel scale 5.93124 arcsec/pix.
Hit/miss: Hit/miss: -+--+--------++-+---+-----+(best)-----+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2459697.solved to indicate this.
Field: out2459697.xyls
Field center: (RA,Dec) = (359.981813, 54.025922) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:55.635, +54:01:33.320).
Field size: 15.6061 x 10.4325 degrees
Field rotation angle: up is 4.46177 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 30 04:26 fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
-rw-r--r-- 1 apache apache 8.5K Jul 30 04:26 out2459697.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat from image00004.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Image size: 926.7'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:55.971 +54:01:36.25 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 14612 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/correct_sextractor_wcs_catalog_usingxy2sky2461211.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1254, bad_region=3331, passed=14612
Got 14612 stars (including 10253 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat
util/solve_plate_with_UCAC5 got 14612 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.1053 through 0 to 14.8809, gap 14.8809 to 345.1053
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3493 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2154 matched stars entering correct_measured_positions(), 2376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2024 matched stars entering correct_measured_positions(), 11767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.96"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.1069 through 0 to 14.8989, gap 14.8989 to 345.1069
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3580 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2403 matched stars entering correct_measured_positions(), 11768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.18"
Accuracy estimation diagnostic: 2322 matched stars entering correct_measured_positions(), 11841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.05"
Excluding outliers - 2322 stars left (next iteration limit 2226)
SIP_REFIT: SIP order 2 trial: matched=2322 robust_rms=26.384 arcsec worst_quadrant_rms=28.915 arcsec
SIP_REFIT: SIP order 3 trial: matched=2322 robust_rms=25.527 arcsec worst_quadrant_rms=29.048 arcsec
SIP_REFIT: SIP order 5 trial: matched=2322 robust_rms=23.296 arcsec worst_quadrant_rms=29.058 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2322 robust_rms_before=31.894 arcsec robust_rms_before_corrected=19.259 arcsec robust_rms_after=26.384 arcsec worst_quadrant_rms_before=24.414 worst_quadrant_rms_after=28.915
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.414 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits N_match=2322 sigma_overall_arcsec=13.571 sigma_q1_arcsec=28.175 sigma_q2_arcsec=27.162 sigma_q3_arcsec=7.081 sigma_q4_arcsec=5.898 n_q1=510 n_q2=269 n_q3=902 n_q4=641 worst_quadrant_to_overall_ratio=2.076
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 2nd new image (fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits): sigma 13.571->13.571, ratio 2.076->2.076; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=13.896 -- 27.38x the reference average (0.5075); plate solution may be of low accuracy
WARNING: 2nd new image has sigma_overall_arcsec=13.571 -- 26.74x the reference average (0.5075); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468_astrometric_residuals.png (4917 matched stars from wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450_astrometric_residuals.png (4912 matched stars from wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416_astrometric_residuals.png (2327 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 12.68 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417_astrometric_residuals.png (2322 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 12.44 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:30.11 +51:36:34.7: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:30.11 +51:36:34.7: 15.46 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out07077.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07077_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 07077_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21482_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 21482_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:44:31.52 +56:34:51.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 15s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:09:30.11 +51:36:34.7
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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.059 +54:00:13.58 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Image size: 926.7'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:58.292 +54:00:51.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.059 +54:00:13.58
Second-epoch image center 23:59:58.292 +54:00:51.92
Angular distance between the image centers 0.0115 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Image size: 926.7'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:55.971 +54:01:36.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.059 +54:00:13.58
Second-epoch image center 23:59:55.971 +54:01:36.25
Angular distance between the image centers 0.0250 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:58.292 +54:00:51.92
Second-epoch second image center 23:59:55.971 +54:01:36.25
Angular distance between the image centers 0.01356 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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.OBsQ80bFbD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.aRsrspOl8y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits &> /tmp/tmp.OMtswLZvDl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits &> /tmp/tmp.5tukFdv7pZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 344.9469 to 14.9293 deg, Dec +48.1259 to +59.2679 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 344.9469 to 14.9293 deg, Dec 48.1259 to 59.2679 deg
Loaded 25504 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): 13217 out of 18826 total matches.
Matched with Tycho-2 18826 out of 200953 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.479600
a=0.000000 b=1.000000 c=22.479600
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 344.9469 to 14.9293 deg, Dec +48.1259 to +59.2679 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 344.9469 to 14.9293 deg, Dec 48.1259 to 59.2679 deg
Loaded 25504 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): 13217 out of 18826 total matches.
Matched with Tycho-2 18826 out of 200953 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=4.7)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 213202 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 344.9557 to 14.9265 deg, Dec +48.1255 to +59.2648 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 344.9557 to 14.9265 deg, Dec 48.1255 to 59.2648 deg
Loaded 25491 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): 12093 out of 17553 total matches.
Matched with Tycho-2 17553 out of 213202 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 201 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.2 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.0 pix fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
2.0 pix fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Limiting magnitude estimates:
15.2 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
15.3 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OBsQ80bFbD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=60, blended=29230, bad_region=30798, passed=200893
Got 200893 stars (including 144443 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 200893 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
RA wraps around 0/360 boundary: field RA 344.9469 through 0 to 14.9293, gap 14.9293 to 344.9469
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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 4923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 178580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9447 through 0 to 14.9298, gap 14.9298 to 344.9447
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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 178580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 178580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4923 stars left (next iteration limit 5415)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=4923 sigma_overall_arcsec=0.484 sigma_q1_arcsec=0.447 sigma_q2_arcsec=0.462 sigma_q3_arcsec=0.519 sigma_q4_arcsec=0.488 n_q1=1437 n_q2=1026 n_q3=1425 n_q4=1035 worst_quadrant_to_overall_ratio=1.073
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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.aRsrspOl8y (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=33709, bad_region=29431, passed=213150
Got 213150 stars (including 154424 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 213150 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
RA wraps around 0/360 boundary: field RA 344.9557 through 0 to 14.9265, gap 14.9265 to 344.9557
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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 4923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 191821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9458 through 0 to 14.9263, gap 14.9263 to 344.9458
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 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 191821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 191821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4922 stars left (next iteration limit 5413)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=4922 sigma_overall_arcsec=0.504 sigma_q1_arcsec=0.458 sigma_q2_arcsec=0.498 sigma_q3_arcsec=0.516 sigma_q4_arcsec=0.534 n_q1=1470 n_q2=988 n_q3=1439 n_q4=1025 worst_quadrant_to_overall_ratio=1.060
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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.OMtswLZvDl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=11032, bad_region=21639, passed=126204
Got 126204 stars (including 95023 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat
util/solve_plate_with_UCAC5 got 126204 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0804 through 0 to 15.0807, gap 15.0807 to 345.0804
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3483 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2146 matched stars entering correct_measured_positions(), 2376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1990 matched stars entering correct_measured_positions(), 109095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0824 through 0 to 15.0995, gap 15.0995 to 345.0824
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3552 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2410 matched stars entering correct_measured_positions(), 109096 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.73"
Accuracy estimation diagnostic: 2330 matched stars entering correct_measured_positions(), 109650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.61"
Excluding outliers - 2330 stars left (next iteration limit 2189)
SIP_REFIT: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits N_match=2330 sigma_overall_arcsec=13.420 sigma_q1_arcsec=28.657 sigma_q2_arcsec=27.998 sigma_q3_arcsec=7.686 sigma_q4_arcsec=5.938 n_q1=514 n_q2=280 n_q3=865 n_q4=671 worst_quadrant_to_overall_ratio=2.135
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.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.5tukFdv7pZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=47, blended=11067, bad_region=21994, passed=127129
Got 127129 stars (including 95588 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat
util/solve_plate_with_UCAC5 got 127129 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0476 through 0 to 15.0763, gap 15.0763 to 345.0476
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3476 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2147 matched stars entering correct_measured_positions(), 2357 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2000 matched stars entering correct_measured_positions(), 109883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.91"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0481 through 0 to 15.0952, gap 15.0952 to 345.0481
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 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3544 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2389 matched stars entering correct_measured_positions(), 109883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.94"
Accuracy estimation diagnostic: 2320 matched stars entering correct_measured_positions(), 110290 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.63"
Excluding outliers - 2320 stars left (next iteration limit 2200)
SIP_REFIT: wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits N_match=2320 sigma_overall_arcsec=13.325 sigma_q1_arcsec=27.675 sigma_q2_arcsec=28.540 sigma_q3_arcsec=7.361 sigma_q4_arcsec=6.119 n_q1=507 n_q2=287 n_q3=866 n_q4=660 worst_quadrant_to_overall_ratio=2.142
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.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_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-00-08_20.00sec_-0.00C_LIGHT_0416.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Cas-04-Q2b1x1_042204_TTUQ2b1x1_2439514_zNGaxFg5/wcs_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:21.89 +53:36:20.5: 15.74 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:19.75 +53:23:15.6: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:52.30 +55:53:13.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:29.57 +53:53:24.0: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:52.89 +53:18:18.1: 15.73 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:03.11 +53:52:00.5: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:05:25.88 +56:42:50.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:42.73 +53:45:27.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:21.89 +53:36:20.5: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:52.89 +53:18:18.1: 15.70 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:19.75 +53:23:15.6: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:29.57 +53:53:24.0: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:59:36.29 +56:58:30.7: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 15.74 +/- 0.34
Forced photometry reference-image weighted average: 15.71 +/- 0.24
Forced photometry filter KEPT candidate at 00:03:21.89 +53:36:20.5: ref_mag=15.74 +/- 0.34 new_mean_mag=14.2502 delta=1.49 (need > 0.90)
Forced photometry filter KEPT candidate at 00:22:52.89 +53:18:18.1: ref_mag=15.71 +/- 0.24 new_mean_mag=14.1735 delta=1.54 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:52.30 +55:53:13.4: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:03.11 +53:52:00.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:05:25.88 +56:42:50.1: 13.43 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:42.73 +53:45:27.4: 15.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter REJECTED candidate at 00:05:25.88 +56:42:50.1: ref_mag=13.39 +/- 0.03 new_mean_mag=14.0517 delta=-0.66 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:36.29 +56:58:30.7: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter REJECTED candidate at 23:59:36.29 +56:58:30.7: ref_mag=13.25 +/- 0.02 new_mean_mag=13.8305 delta=-0.58 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:17:03.71 +57:24:10.4: 13.71 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:17:03.71 +57:24:10.4: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter REJECTED candidate at 00:17:03.71 +57:24:10.4: ref_mag=13.75 +/- 0.04 new_mean_mag=13.8416 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:18.97 +55:00:40.0: 14.73 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:58.19 +52:48:56.6: 15.32 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:18.97 +55:00:40.0: 14.70 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.09
Forced photometry filter REJECTED candidate at 00:11:18.97 +55:00:40.0: ref_mag=14.71 +/- 0.09 new_mean_mag=14.0078 delta=0.70 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:59.93 +52:33:28.9: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:58.19 +52:48:56.6: 15.95 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.32 +/- 0.22
Forced photometry filter KEPT candidate at 00:10:58.19 +52:48:56.6: ref_mag=15.32 +/- 0.22 new_mean_mag=13.9069 delta=1.41 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:59.93 +52:33:28.9: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:08:33.77 +55:38:51.9: 13.31 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:33.77 +55:38:51.9: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter REJECTED candidate at 00:08:33.77 +55:38:51.9: ref_mag=13.38 +/- 0.03 new_mean_mag=13.6617 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:48.63 +53:58:07.0: 15.51 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:48.63 +53:58:07.0: 15.16 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.16
Forced photometry filter KEPT candidate at 00:12:48.63 +53:58:07.0: ref_mag=15.28 +/- 0.16 new_mean_mag=13.8331 delta=1.44 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:32.06 +52:54:22.9: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:32.06 +52:54:22.9: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:09.80 +51:29:13.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:09.80 +51:29:13.7: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:28:05.45 +53:55:26.5: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:28:05.45 +53:55:26.5: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:40.19 +55:18:36.6: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:40.19 +55:18:36.6: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:27:40.62 +55:49:21.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:11.10 +50:58:17.2: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:40.62 +55:49:21.0: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:27.39 +51:58:26.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:40.48 +57:10:20.8: 13.46 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:11.10 +50:58:17.2: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:33.00 +55:49:44.8: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:40.48 +57:10:20.8: 13.41 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:27.39 +51:58:26.2: 16.00 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter REJECTED candidate at 23:55:40.48 +57:10:20.8: ref_mag=13.43 +/- 0.03 new_mean_mag=13.6705 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:33.00 +55:49:44.8: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter REJECTED candidate at 00:30:33.00 +55:49:44.8: ref_mag=12.33 +/- 0.01 new_mean_mag=13.7222 delta=-1.39 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:27.20 +52:39:45.1: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:21.62 +55:27:42.1: 14.26 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:58.21 +56:09:24.3: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:27.20 +52:39:45.1: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:21.62 +55:27:42.1: 14.27 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.07
Forced photometry filter REJECTED candidate at 00:24:21.62 +55:27:42.1: ref_mag=14.27 +/- 0.07 new_mean_mag=13.6314 delta=0.63 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:58.21 +56:09:24.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter REJECTED candidate at 23:52:58.21 +56:09:24.3: ref_mag=13.17 +/- 0.02 new_mean_mag=13.6332 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:27:01.50 +51:15:17.1: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:01.50 +51:15:17.1: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:34.67 +57:42:53.3: 13.34 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:34.67 +57:42:53.3: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter REJECTED candidate at 23:46:34.67 +57:42:53.3: ref_mag=13.38 +/- 0.03 new_mean_mag=13.6817 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:44.40 +53:20:10.7: 15.68 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:44.40 +53:20:10.7: 15.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.68 +/- 0.33
Forced photometry filter KEPT candidate at 00:03:44.40 +53:20:10.7: ref_mag=15.68 +/- 0.33 new_mean_mag=13.5887 delta=2.09 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:39.88 +56:54:31.0: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:39.88 +56:54:31.0: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:43.74 +54:49:49.8: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:43.74 +54:49:49.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:59.18 +56:58:33.6: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:59.18 +56:58:33.6: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:54.23 +51:47:15.9: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:54.23 +51:47:15.9: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:28.25 +56:13:36.7: 13.09 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:28.25 +56:13:36.7: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter REJECTED candidate at 23:56:28.25 +56:13:36.7: ref_mag=13.04 +/- 0.02 new_mean_mag=13.2834 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:08:21.64 +52:43:31.0: 14.40 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:09.42 +54:36:39.8: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:22.96 +56:28:07.3: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:21.64 +52:43:31.0: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry filter REJECTED candidate at 00:08:21.64 +52:43:31.0: ref_mag=13.92 +/- 0.05 new_mean_mag=13.3591 delta=0.56 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:09.42 +54:36:39.8: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:22.96 +56:28:07.3: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:35.99 +50:40:52.8: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:35.99 +50:40:52.8: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:40.88 +56:24:45.3: 12.84 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:40.88 +56:24:45.3: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Forced photometry filter REJECTED candidate at 23:56:40.88 +56:24:45.3: ref_mag=12.77 +/- 0.02 new_mean_mag=13.3476 delta=-0.58 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:56.88 +57:43:33.4: 12.99 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:17.74 +55:33:35.7: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:56.88 +57:43:33.4: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter REJECTED candidate at 00:31:56.88 +57:43:33.4: ref_mag=13.02 +/- 0.02 new_mean_mag=13.1071 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:05.07 +54:12:31.8: 15.49 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:17.74 +55:33:35.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:05.07 +54:12:31.8: 15.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.49 +/- 0.31
Forced photometry filter KEPT candidate at 23:55:05.07 +54:12:31.8: ref_mag=15.49 +/- 0.31 new_mean_mag=13.2238 delta=2.27 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:21:31.83 +50:34:21.8: 14.18 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:21:31.83 +50:34:21.8: 14.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.06
Forced photometry filter KEPT candidate at 00:21:31.83 +50:34:21.8: ref_mag=14.27 +/- 0.06 new_mean_mag=13.2253 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:21:11.81 +54:40:22.6: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:38.21 +57:54:59.4: 12.95 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:21:11.81 +54:40:22.6: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:38.21 +57:54:59.4: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter REJECTED candidate at 00:30:38.21 +57:54:59.4: ref_mag=13.00 +/- 0.02 new_mean_mag=13.1786 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:51.05 +55:31:01.4: 15.72 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:09.22 +53:39:27.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:27.07 +56:43:29.1: 14.77 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:51.05 +55:31:01.4: 15.37 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.47 +/- 0.19
Forced photometry filter KEPT candidate at 00:23:51.05 +55:31:01.4: ref_mag=15.47 +/- 0.19 new_mean_mag=13.1838 delta=2.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:09.22 +53:39:27.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:27.07 +56:43:29.1: 14.98 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.11
Forced photometry filter KEPT candidate at 00:14:27.07 +56:43:29.1: ref_mag=14.86 +/- 0.11 new_mean_mag=13.0553 delta=1.81 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:35.40 +57:13:31.0: 14.53 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:35.40 +57:13:31.0: 14.55 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.09
Forced photometry filter KEPT candidate at 23:28:35.40 +57:13:31.0: ref_mag=14.54 +/- 0.09 new_mean_mag=13.1482 delta=1.39 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:38.59 +53:55:16.3: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:38.59 +53:55:16.3: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:27.03 +55:56:11.2: 15.00 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:26.74 +50:05:20.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:15.61 +55:46:37.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:27.03 +55:56:11.2: 15.20 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.13
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:26.74 +50:05:20.1: 15.88 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 00:30:27.03 +55:56:11.2: ref_mag=15.09 +/- 0.13 new_mean_mag=12.9200 delta=2.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:15.61 +55:46:37.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:17.54 +54:44:27.9: 15.04 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:17.54 +54:44:27.9: 14.69 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.11
Forced photometry filter KEPT candidate at 00:06:17.54 +54:44:27.9: ref_mag=14.80 +/- 0.11 new_mean_mag=13.0254 delta=1.77 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:22.38 +56:52:26.2: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:22.38 +56:52:26.2: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:47.94 +52:07:06.0: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:47.94 +52:07:06.0: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:47.04 +57:10:52.9: 12.30 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:47.04 +57:10:52.9: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter REJECTED candidate at 23:54:47.04 +57:10:52.9: ref_mag=12.20 +/- 0.01 new_mean_mag=12.7854 delta=-0.58 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:17:52.88 +57:46:39.4: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:08.26 +54:51:02.0: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:17:52.88 +57:46:39.4: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry filter REJECTED candidate at 00:17:52.88 +57:46:39.4: ref_mag=12.68 +/- 0.02 new_mean_mag=12.7948 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:02.14 +53:09:42.5: 12.84 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:08.26 +54:51:02.0: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:02.14 +53:09:42.5: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter REJECTED candidate at 23:52:02.14 +53:09:42.5: ref_mag=12.84 +/- 0.02 new_mean_mag=12.7061 delta=0.13 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:37.45 +56:53:36.6: 10.65 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:24.04 +57:11:29.8: 12.30 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:37.45 +56:53:36.6: 10.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.74 +/- 0.00
Forced photometry filter REJECTED candidate at 00:13:37.45 +56:53:36.6: ref_mag=10.74 +/- 0.00 new_mean_mag=12.5361 delta=-1.80 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:24.04 +57:11:29.8: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter REJECTED candidate at 00:24:24.04 +57:11:29.8: ref_mag=12.32 +/- 0.01 new_mean_mag=12.5080 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:48.86 +52:27:47.7: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:48.86 +52:27:47.7: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:00.15 +51:35:37.6: 14.12 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:10.33 +53:13:09.0: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:00.15 +51:35:37.6: 14.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.06
Forced photometry filter KEPT candidate at 00:14:00.15 +51:35:37.6: ref_mag=14.20 +/- 0.06 new_mean_mag=11.7966 delta=2.40 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:10.33 +53:13:09.0: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:20.52 +55:49:18.3: 14.82 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:20.52 +55:49:18.3: 14.48 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.11
Forced photometry filter KEPT candidate at 00:23:20.52 +55:49:18.3: ref_mag=14.59 +/- 0.11 new_mean_mag=12.9954 delta=1.59 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:01.28 +50:30:16.1: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:01.28 +50:30:16.1: 15.21 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.23
Forced photometry filter KEPT candidate at 23:58:01.28 +50:30:16.1: ref_mag=15.21 +/- 0.23 new_mean_mag=12.9943 delta=2.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:56.07 +56:28:26.1: 12.81 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:56.07 +56:28:26.1: 12.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Forced photometry filter REJECTED candidate at 23:57:56.07 +56:28:26.1: ref_mag=12.80 +/- 0.03 new_mean_mag=13.0950 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:02.57 +50:09:43.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:02.57 +50:09:43.6: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:59.98 +50:31:00.1: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:59.98 +50:31:00.1: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:48.07 +53:02:40.7: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:48.07 +53:02:40.7: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:30.03 +53:45:20.0: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:30.03 +53:45:20.0: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:45.39 +52:44:43.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:45.39 +52:44:43.4: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:54.65 +50:00:36.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:54.65 +50:00:36.7: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:17.18 +50:18:36.8: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:17.18 +50:18:36.8: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:59:00.94 +53:17:41.6: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:00.94 +53:17:41.6: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:27.68 +57:57:21.2: 13.74 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:27.68 +57:57:21.2: 13.77 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.05
Forced photometry filter REJECTED candidate at 23:30:27.68 +57:57:21.2: ref_mag=13.76 +/- 0.05 new_mean_mag=13.3138 delta=0.44 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:00.96 +53:37:01.0: 14.28 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:00.96 +53:37:01.0: 14.53 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.08
Forced photometry filter KEPT candidate at 00:12:00.96 +53:37:01.0: ref_mag=14.39 +/- 0.08 new_mean_mag=13.4064 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:13.81 +55:08:27.8: 13.55 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:13.81 +55:08:27.8: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter REJECTED candidate at 23:57:13.81 +55:08:27.8: ref_mag=13.55 +/- 0.03 new_mean_mag=13.4218 delta=0.13 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:16.25 +55:19:37.7: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:16.25 +55:19:37.7: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:54.20 +56:29:17.2: 13.13 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:54.20 +56:29:17.2: 13.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.05
Forced photometry filter REJECTED candidate at 23:57:54.20 +56:29:17.2: ref_mag=13.15 +/- 0.05 new_mean_mag=13.4411 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:55.48 +53:41:36.5: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:55.48 +53:41:36.5: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:41.40 +56:26:52.0: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:41.40 +56:26:52.0: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:24.80 +57:49:21.2: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:24.80 +57:49:21.2: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:50.25 +55:37:38.0: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:50.25 +55:37:38.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:54.18 +55:16:27.8: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:54.18 +55:16:27.8: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:38.02 +50:48:48.7: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:38.02 +50:48:48.7: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:27:12.05 +54:06:10.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:12.05 +54:06:10.9: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:40.28 +57:11:18.3: 13.89 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:40.28 +57:11:18.3: 13.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.06
Forced photometry filter REJECTED candidate at 00:07:40.28 +57:11:18.3: ref_mag=13.58 +/- 0.06 new_mean_mag=13.6749 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:27.85 +55:39:35.2: 13.41 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:27.85 +55:39:35.2: 13.36 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Forced photometry filter REJECTED candidate at 00:03:27.85 +55:39:35.2: ref_mag=13.38 +/- 0.04 new_mean_mag=13.6133 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:58.20 +54:11:17.1: 14.51 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:26.63 +54:13:52.6: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:58.20 +54:11:17.1: 14.87 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.14
Forced photometry filter REJECTED candidate at 23:31:58.20 +54:11:17.1: ref_mag=14.64 +/- 0.14 new_mean_mag=13.8471 delta=0.79 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:01.37 +54:43:38.9: 13.33 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:26.63 +54:13:52.6: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:51:01.37 +54:43:38.9: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter REJECTED candidate at 23:51:01.37 +54:43:38.9: ref_mag=13.32 +/- 0.03 new_mean_mag=13.8009 delta=-0.48 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:22.17 +53:19:57.7: 14.52 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:22.17 +53:19:57.7: 14.92 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.10
Forced photometry filter KEPT candidate at 00:24:22.17 +53:19:57.7: ref_mag=14.69 +/- 0.10 new_mean_mag=13.7175 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:57.22 +54:41:07.9: 14.03 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:57.22 +54:41:07.9: 14.04 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Forced photometry filter REJECTED candidate at 23:41:57.22 +54:41:07.9: ref_mag=14.03 +/- 0.06 new_mean_mag=13.7934 delta=0.24 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:34.07 +55:55:46.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:34.07 +55:55:46.4: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:39.23 +55:00:08.6: 14.07 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:39.23 +55:00:08.6: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Forced photometry filter REJECTED candidate at 23:57:39.23 +55:00:08.6: ref_mag=14.02 +/- 0.05 new_mean_mag=13.8588 delta=0.16 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:48.56 +55:50:46.5: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:48.56 +55:50:46.5: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:05.94 +53:56:13.3: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:51:05.94 +53:56:13.3: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:21:15.51 +56:23:24.0: 14.76 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:21:15.51 +56:23:24.0: 14.99 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.12
Forced photometry filter REJECTED candidate at 00:21:15.51 +56:23:24.0: ref_mag=14.87 +/- 0.12 new_mean_mag=14.0405 delta=0.83 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:48:20.07 +54:53:19.8: 13.93 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:48:20.07 +54:53:19.8: 13.99 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.06
Forced photometry filter REJECTED candidate at 23:48:20.07 +54:53:19.8: ref_mag=13.96 +/- 0.06 new_mean_mag=14.0946 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:28.86 +55:39:03.7: 14.06 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:31.39 +54:58:29.6: 14.05 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:28.86 +55:39:03.7: 14.09 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.07
Forced photometry filter REJECTED candidate at 00:03:28.86 +55:39:03.7: ref_mag=14.07 +/- 0.07 new_mean_mag=13.9013 delta=0.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:31.39 +54:58:29.6: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Forced photometry filter REJECTED candidate at 23:54:31.39 +54:58:29.6: ref_mag=14.05 +/- 0.05 new_mean_mag=14.0569 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:01.52 +52:37:15.8: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:01.52 +52:37:15.8: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:11.85 +54:17:11.6: 15.43 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:42.35 +50:06:37.3: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:43.39 +54:46:57.7: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:42.35 +50:06:37.3: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:11.85 +54:17:11.6: 15.60 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.51 +/- 0.23
Forced photometry filter KEPT candidate at 00:04:11.85 +54:17:11.6: ref_mag=15.51 +/- 0.23 new_mean_mag=13.4423 delta=2.07 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:43.39 +54:46:57.7: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:23.05 +52:35:46.6: 13.98 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:23.05 +52:35:46.6: 14.21 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.08
Forced photometry filter REJECTED candidate at 00:02:23.05 +52:35:46.6: ref_mag=14.09 +/- 0.08 new_mean_mag=13.2404 delta=0.85 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out235720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out100500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25587.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 104s
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: 46s
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Considering the candidate 235424_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235424_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 235435_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235435_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235453_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235453_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235465_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235465_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 235466_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235466_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235473_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235473_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235477_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235477_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235479_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235479_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235481_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235481_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 235491_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235491_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 235493_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235493_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235495_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235495_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
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Considering the candidate 235502_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235502_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
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Considering the candidate 235503_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235503_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 235507_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235507_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 235510_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235510_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
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Considering the candidate 235517_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235517_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 235529_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235529_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
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Considering the candidate 235533_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235533_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235534_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235534_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235536_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235536_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 235538_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235538_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:21:58.93 +57:17:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235540_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235540_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
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Considering the candidate 235542_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235542_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 235546_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235546_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 235548_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235548_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 235552_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235552_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235558_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235558_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 235561_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235561_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235570_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235570_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 235572_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235572_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235581_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235581_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235584_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235584_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 235590_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235590_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235596_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235596_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 235598_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235598_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235599_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235599_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:56:55.55 +55:04:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235601_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235601_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 235605_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235605_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235607_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235607_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
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Considering the candidate 235610_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235610_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 235613_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235613_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
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Considering the candidate 235614_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235614_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235615_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235615_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235617_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235617_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235619_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235619_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235626_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235626_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235630_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235630_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 235632_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235632_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235633_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235633_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (34.4") between the two second-epoch detections
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Considering the candidate 235639_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235639_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 235641_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235641_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 235644_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235644_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 235649_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235649_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235651_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235651_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 235652_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235652_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 235654_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235654_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235658_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235658_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 235661_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235661_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235666_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235666_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235671_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235671_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235674_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235674_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 235676_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235676_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235677_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235677_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 235680_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235680_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235681_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235681_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235683_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235683_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235686_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235686_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:56:59.86 +56:44:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235687_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235687_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235689_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235689_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 235692_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235692_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 235701_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235701_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235703_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235703_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 235704_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235704_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235705_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:57:15.99 +56:30:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235707_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235707_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 235710_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235710_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235711_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235711_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 235713_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235713_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235716_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235716_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235720_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235720_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:21:31.83 +50:34:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.789 394725984340161920 005.38310378357 +50.57232922258 14.0118 13.3068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235721_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235721_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235726_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235726_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235729_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235729_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235730_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235730_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:57:55.28 +56:42:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235734_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235734_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235737_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235737_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235738_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235738_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235740_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235740_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235744_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235744_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:06:20.80 +56:11:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235745_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235745_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235746_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235746_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 235748_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235748_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235749_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235749_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235750_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235750_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235753_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235753_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235755_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235755_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235756_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235756_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235763_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235763_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235764_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235764_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235765_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235765_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235767_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235767_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235769_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235769_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235770_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235770_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235771_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235771_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235774_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235774_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235781_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235781_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235783_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235783_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235791_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235791_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235792_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235792_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235795_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235795_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235837_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235837_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 235902_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235902_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 235912_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235912_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:42:05.33 +57:16:06.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235913_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235913_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:43:56.73 +56:20:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235914_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235914_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:54:36.41 +57:28:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235925_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235925_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:47:14.76 +57:25:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235929_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235929_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:42:06.72 +57:15:36.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235947_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235947_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 235953_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235953_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 235961_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235961_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:25:45.90 +57:58:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235966_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235966_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235968_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235968_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 235975_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235975_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235976_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235976_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 235981_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235981_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 235988_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235988_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
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Considering the candidate 235998_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 235998_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235999_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 235999_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 236000_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236000_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 236014_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236014_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236015_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236015_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 236025_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236025_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:58:51.54 +54:42:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236031_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236031_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236036_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236036_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:25:48.48 +57:59:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236041_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236041_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236050_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236050_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 236058_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236058_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236063_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236063_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236067_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236067_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 236070_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236070_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236071_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236071_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236072_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236072_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236079_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236079_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
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Considering the candidate 236080_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236080_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236085_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236085_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236088_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236088_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:49:47.04 +56:38:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236089_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236089_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236094_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236094_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236098_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236098_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:53:43.32 +56:48:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236105_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236105_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236107_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236107_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236112_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236112_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236115_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236115_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236117_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236117_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236123_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236123_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:00:23.22 +56:50:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236126_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236126_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236130_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236130_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:31:16.92 +57:14:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236132_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236132_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236137_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236137_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236141_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236141_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:20:15.63 +57:50:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236145_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236145_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236149_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236149_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236151_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236151_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236157_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236157_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236159_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236159_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236163_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236163_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236168_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236168_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236175_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236175_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236176_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236176_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236178_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236178_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236187_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236187_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236188_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236188_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236191_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236191_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236192_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236192_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236197_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236197_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236207_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236207_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236209_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236209_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:44:19.94 +57:20:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236221_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236221_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (62.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236231_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236231_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236237_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236237_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236242_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236242_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236248_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236248_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236249_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236249_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236251_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236251_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:02:26.66 +54:33:00.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236258_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236258_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236271_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236271_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236279_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236279_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236280_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236280_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236291_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236291_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236301_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236301_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236307_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 236307_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236311_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 236311_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121532_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 121532_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100500_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
Preparing report for the candidate 100500_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191364_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 191364_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:59:54.33 +56:58:43.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179100_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 179100_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 00:15:50.70 +57:32:35.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197606_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 197606_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
**** FOUND 23:44:32.03 +56:34:51.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46841_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 46841_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64302_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417
The candidate 64302_fd_Cas-04-Q2b1x1_2026-07-30_04-01-05_20.00sec_-0.00C_LIGHT_0417 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 155s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:09:30.11 +51:36:34.7
00:04:11.85 +54:17:11.6
23:20:43.39 +54:46:57.7
00:10:19.75 +53:23:15.6
00:03:21.89 +53:36:20.5
00:12:52.30 +55:53:13.4
00:11:29.57 +53:53:24.0
00:22:52.89 +53:18:18.1
00:20:03.11 +53:52:00.5
00:00:42.73 +53:45:27.4
00:10:58.19 +52:48:56.6
00:11:59.93 +52:33:28.9
00:12:48.63 +53:58:07.0
00:04:32.06 +52:54:22.9
00:12:09.80 +51:29:13.7
00:28:05.45 +53:55:26.5
23:39:40.19 +55:18:36.6
00:27:40.62 +55:49:21.0
00:10:11.10 +50:58:17.2
23:52:27.39 +51:58:26.2
00:25:27.20 +52:39:45.1
00:27:01.50 +51:15:17.1
00:03:44.40 +53:20:10.7
23:31:39.88 +56:54:31.0
00:11:43.74 +54:49:49.8
23:36:59.18 +56:58:33.6
00:20:54.23 +51:47:15.9
23:22:09.42 +54:36:39.8
00:24:22.96 +56:28:07.3
23:28:35.99 +50:40:52.8
00:30:17.74 +55:33:35.7
23:55:05.07 +54:12:31.8
00:21:11.81 +54:40:22.6
00:23:51.05 +55:31:01.4
00:25:09.22 +53:39:27.9
00:14:27.07 +56:43:29.1
23:28:35.40 +57:13:31.0
23:58:38.59 +53:55:16.3
00:30:27.03 +55:56:11.2
23:55:26.74 +50:05:20.1
00:26:15.61 +55:46:37.8
00:06:17.54 +54:44:27.9
23:10:22.38 +56:52:26.2
00:25:47.94 +52:07:06.0
23:22:08.26 +54:51:02.0
00:13:48.86 +52:27:47.7
00:14:00.15 +51:35:37.6
00:15:10.33 +53:13:09.0
00:23:20.52 +55:49:18.3
23:58:01.28 +50:30:16.1
00:20:02.57 +50:09:43.6
23:57:59.98 +50:31:00.1
00:24:48.07 +53:02:40.7
23:56:30.03 +53:45:20.0
23:33:45.39 +52:44:43.4
00:12:54.65 +50:00:36.7
23:55:17.18 +50:18:36.8
23:59:00.94 +53:17:41.6
00:12:00.96 +53:37:01.0
23:12:16.25 +55:19:37.7
00:07:55.48 +53:41:36.5
00:22:41.40 +56:26:52.0
23:28:24.80 +57:49:21.2
23:19:50.25 +55:37:38.0
00:13:54.18 +55:16:27.8
00:19:38.02 +50:48:48.7
00:27:12.05 +54:06:10.9
23:50:26.63 +54:13:52.6
00:24:22.17 +53:19:57.7
23:21:34.07 +55:55:46.4
00:12:48.56 +55:50:46.5
23:51:05.94 +53:56:13.3
00:02:01.52 +52:37:15.8
23:21:42.35 +50:06:37.3
########### Completed Cas-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
00:09:30.11 +51:36:34.7
00:10:19.75 +53:23:15.6
00:03:21.89 +53:36:20.5
00:12:52.30 +55:53:13.4
00:11:29.57 +53:53:24.0
00:22:52.89 +53:18:18.1
00:20:03.11 +53:52:00.5
00:00:42.73 +53:45:27.4
00:10:58.19 +52:48:56.6
00:11:59.93 +52:33:28.9
00:12:48.63 +53:58:07.0
00:04:32.06 +52:54:22.9
00:12:09.80 +51:29:13.7
00:28:05.45 +53:55:26.5
23:39:40.19 +55:18:36.6
00:27:40.62 +55:49:21.0
00:10:11.10 +50:58:17.2
23:52:27.39 +51:58:26.2
00:25:27.20 +52:39:45.1
00:27:01.50 +51:15:17.1
00:03:44.40 +53:20:10.7
23:31:39.88 +56:54:31.0
00:11:43.74 +54:49:49.8
23:36:59.18 +56:58:33.6
00:20:54.23 +51:47:15.9
23:22:09.42 +54:36:39.8
00:24:22.96 +56:28:07.3
23:28:35.99 +50:40:52.8
00:30:17.74 +55:33:35.7
23:55:05.07 +54:12:31.8
00:21:11.81 +54:40:22.6
00:23:51.05 +55:31:01.4
00:25:09.22 +53:39:27.9
00:14:27.07 +56:43:29.1
23:28:35.40 +57:13:31.0
23:58:38.59 +53:55:16.3
00:30:27.03 +55:56:11.2
23:55:26.74 +50:05:20.1
00:26:15.61 +55:46:37.8
00:06:17.54 +54:44:27.9
23:10:22.38 +56:52:26.2
00:25:47.94 +52:07:06.0
23:22:08.26 +54:51:02.0
00:13:48.86 +52:27:47.7
00:14:00.15 +51:35:37.6
00:15:10.33 +53:13:09.0
00:23:20.52 +55:49:18.3
23:58:01.28 +50:30:16.1
00:20:02.57 +50:09:43.6
23:57:59.98 +50:31:00.1
00:24:48.07 +53:02:40.7
23:56:30.03 +53:45:20.0
23:33:45.39 +52:44:43.4
00:12:54.65 +50:00:36.7
23:55:17.18 +50:18:36.8
23:59:00.94 +53:17:41.6
00:12:00.96 +53:37:01.0
23:12:16.25 +55:19:37.7
00:07:55.48 +53:41:36.5
00:22:41.40 +56:26:52.0
23:28:24.80 +57:49:21.2
23:19:50.25 +55:37:38.0
00:13:54.18 +55:16:27.8
00:19:38.02 +50:48:48.7
00:27:12.05 +54:06:10.9
23:50:26.63 +54:13:52.6
00:24:22.17 +53:19:57.7
23:21:34.07 +55:55:46.4
00:12:48.56 +55:50:46.5
23:51:05.94 +53:56:13.3
00:02:01.52 +52:37:15.8
23:20:43.39 +54:46:57.7
23:21:42.35 +50:06:37.3
00:04:11.85 +54:17:11.6
###################################################################################
00:09:30.11 +51:36:34.7 -- not an asteroid (will add it to exclusion list)
00:10:19.75 +53:23:15.6 -- not an asteroid (will add it to exclusion list)
00:03:21.89 +53:36:20.5 -- not an asteroid (will add it to exclusion list)
00:12:52.30 +55:53:13.4 -- not an asteroid (will add it to exclusion list)
00:11:29.57 +53:53:24.0 -- not an asteroid (will add it to exclusion list)
00:22:52.89 +53:18:18.1 -- not an asteroid (will add it to exclusion list)
00:20:03.11 +53:52:00.5 -- not an asteroid (will add it to exclusion list)
00:00:42.73 +53:45:27.4 -- not an asteroid (will add it to exclusion list)
00:10:58.19 +52:48:56.6 -- not an asteroid (will add it to exclusion list)
00:11:59.93 +52:33:28.9 -- not an asteroid (will add it to exclusion list)
00:12:48.63 +53:58:07.0 -- not an asteroid (will add it to exclusion list)
00:04:32.06 +52:54:22.9 -- not an asteroid (will add it to exclusion list)
00:12:09.80 +51:29:13.7 -- not an asteroid (will add it to exclusion list)
00:28:05.45 +53:55:26.5 -- not an asteroid (will add it to exclusion list)
23:39:40.19 +55:18:36.6 -- not an asteroid (will add it to exclusion list)
00:27:40.62 +55:49:21.0 -- not an asteroid (will add it to exclusion list)
00:10:11.10 +50:58:17.2 -- not an asteroid (will add it to exclusion list)
23:52:27.39 +51:58:26.2 -- not an asteroid (will add it to exclusion list)
00:25:27.20 +52:39:45.1 -- not an asteroid (will add it to exclusion list)
00:27:01.50 +51:15:17.1 -- not an asteroid (will add it to exclusion list)
00:03:44.40 +53:20:10.7 -- not an asteroid (will add it to exclusion list)
23:31:39.88 +56:54:31.0 -- not an asteroid (will add it to exclusion list)
00:11:43.74 +54:49:49.8 -- not an asteroid (will add it to exclusion list)
23:36:59.18 +56:58:33.6 -- not an asteroid (will add it to exclusion list)
00:20:54.23 +51:47:15.9 -- not an asteroid (will add it to exclusion list)
23:22:09.42 +54:36:39.8 -- not an asteroid (will add it to exclusion list)
00:24:22.96 +56:28:07.3 -- not an asteroid (will add it to exclusion list)
23:28:35.99 +50:40:52.8 -- not an asteroid (will add it to exclusion list)
00:30:17.74 +55:33:35.7 -- not an asteroid (will add it to exclusion list)
23:55:05.07 +54:12:31.8 -- not an asteroid (will add it to exclusion list)
00:21:11.81 +54:40:22.6 -- not an asteroid (will add it to exclusion list)
00:23:51.05 +55:31:01.4 -- not an asteroid (will add it to exclusion list)
00:25:09.22 +53:39:27.9 -- not an asteroid (will add it to exclusion list)
00:14:27.07 +56:43:29.1 -- not an asteroid (will add it to exclusion list)
23:28:35.40 +57:13:31.0 -- not an asteroid (will add it to exclusion list)
23:58:38.59 +53:55:16.3 -- not an asteroid (will add it to exclusion list)
00:30:27.03 +55:56:11.2 -- not an asteroid (will add it to exclusion list)
23:55:26.74 +50:05:20.1 -- not an asteroid (will add it to exclusion list)
00:26:15.61 +55:46:37.8 -- not an asteroid (will add it to exclusion list)
00:06:17.54 +54:44:27.9 -- not an asteroid (will add it to exclusion list)
23:10:22.38 +56:52:26.2 -- not an asteroid (will add it to exclusion list)
00:25:47.94 +52:07:06.0 -- not an asteroid (will add it to exclusion list)
23:22:08.26 +54:51:02.0 -- not an asteroid (will add it to exclusion list)
00:13:48.86 +52:27:47.7 -- not an asteroid (will add it to exclusion list)
00:14:00.15 +51:35:37.6 -- not an asteroid (will add it to exclusion list)
00:15:10.33 +53:13:09.0 -- not an asteroid (will add it to exclusion list)
00:23:20.52 +55:49:18.3 -- not an asteroid (will add it to exclusion list)
23:58:01.28 +50:30:16.1 -- not an asteroid (will add it to exclusion list)
00:20:02.57 +50:09:43.6 -- not an asteroid (will add it to exclusion list)
23:57:59.98 +50:31:00.1 -- not an asteroid (will add it to exclusion list)
00:24:48.07 +53:02:40.7 -- not an asteroid (will add it to exclusion list)
23:56:30.03 +53:45:20.0 -- not an asteroid (will add it to exclusion list)
23:33:45.39 +52:44:43.4 -- not an asteroid (will add it to exclusion list)
00:12:54.65 +50:00:36.7 -- not an asteroid (will add it to exclusion list)
23:55:17.18 +50:18:36.8 -- not an asteroid (will add it to exclusion list)
23:59:00.94 +53:17:41.6 -- not an asteroid (will add it to exclusion list)
00:12:00.96 +53:37:01.0 -- not an asteroid (will add it to exclusion list)
23:12:16.25 +55:19:37.7 -- not an asteroid (will add it to exclusion list)
00:07:55.48 +53:41:36.5 -- not an asteroid (will add it to exclusion list)
00:22:41.40 +56:26:52.0 -- not an asteroid (will add it to exclusion list)
23:28:24.80 +57:49:21.2 -- not an asteroid (will add it to exclusion list)
23:19:50.25 +55:37:38.0 -- not an asteroid (will add it to exclusion list)
00:13:54.18 +55:16:27.8 -- not an asteroid (will add it to exclusion list)
00:19:38.02 +50:48:48.7 -- not an asteroid (will add it to exclusion list)
00:27:12.05 +54:06:10.9 -- not an asteroid (will add it to exclusion list)
23:50:26.63 +54:13:52.6 -- not an asteroid (will add it to exclusion list)
00:24:22.17 +53:19:57.7 -- not an asteroid (will add it to exclusion list)
23:21:34.07 +55:55:46.4 -- not an asteroid (will add it to exclusion list)
00:12:48.56 +55:50:46.5 -- not an asteroid (will add it to exclusion list)
23:51:05.94 +53:56:13.3 -- not an asteroid (will add it to exclusion list)
00:02:01.52 +52:37:15.8 -- not an asteroid (will add it to exclusion list)
23:20:43.39 +54:46:57.7 -- not an asteroid (will add it to exclusion list)
23:21:42.35 +50:06:37.3 -- not an asteroid (will add it to exclusion list)
00:04:11.85 +54:17:11.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:42.73 +53:45:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:01.52 +52:37:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:21.89 +53:36:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:44.40 +53:20:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:11.85 +54:17:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:32.06 +52:54:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:17.54 +54:44:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:55.48 +53:41:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:30.11 +51:36:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:11.10 +50:58:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:19.75 +53:23:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:58.19 +52:48:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:29.57 +53:53:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:43.74 +54:49:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:59.93 +52:33:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:00.96 +53:37:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:09.80 +51:29:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:48.56 +55:50:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:48.63 +53:58:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:52.30 +55:53:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:54.65 +50:00:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:48.86 +52:27:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:54.18 +55:16:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:00.15 +51:35:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:27.07 +56:43:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:10.33 +53:13:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:38.02 +50:48:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:02.57 +50:09:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:03.11 +53:52:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:54.23 +51:47:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:11.81 +54:40:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:41.40 +56:26:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:52.89 +53:18:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:20.52 +55:49:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:51.05 +55:31:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:22.17 +53:19:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:22.96 +56:28:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:48.07 +53:02:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:09.22 +53:39:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:27.20 +52:39:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:47.94 +52:07:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:15.61 +55:46:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:01.50 +51:15:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:12.05 +54:06:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:40.62 +55:49:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:05.45 +53:55:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:17.74 +55:33:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:27.03 +55:56:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:22.38 +56:52:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:16.25 +55:19:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:50.25 +55:37:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:43.39 +54:46:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:34.07 +55:55:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:42.35 +50:06:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:08.26 +54:51:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:09.42 +54:36:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:24.80 +57:49:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:35.40 +57:13:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:35.99 +50:40:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:39.88 +56:54:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:45.39 +52:44:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:59.18 +56:58:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:40.19 +55:18:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:26.63 +54:13:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:05.94 +53:56:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:27.39 +51:58:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:05.07 +54:12:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:17.18 +50:18:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:26.74 +50:05:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:30.03 +53:45:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:59.98 +50:31:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:01.28 +50:30:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:38.59 +53:55:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:00.94 +53:17:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:00:42.73 +53:45:27.4 -- not a known variable star
00:02:01.52 +52:37:15.8 -- not a known variable star
00:03:21.89 +53:36:20.5 -- not a known variable star
00:03:44.40 +53:20:10.7 -- a known variable star
00:04:11.85 +54:17:11.6 -- not a known variable star
00:04:32.06 +52:54:22.9 -- not a known variable star
00:06:17.54 +54:44:27.9 -- a known variable star
00:07:55.48 +53:41:36.5 -- a known variable star
00:09:30.11 +51:36:34.7 -- not a known variable star
00:10:11.10 +50:58:17.2 -- not a known variable star
00:10:19.75 +53:23:15.6 -- a known variable star
00:10:58.19 +52:48:56.6 -- not a known variable star
00:11:29.57 +53:53:24.0 -- not a known variable star
00:11:43.74 +54:49:49.8 -- not a known variable star
00:11:59.93 +52:33:28.9 -- not a known variable star
00:12:00.96 +53:37:01.0 -- not a known variable star
00:12:09.80 +51:29:13.7 -- not a known variable star
00:12:48.56 +55:50:46.5 -- not a known variable star
00:12:48.63 +53:58:07.0 -- not a known variable star
00:12:52.30 +55:53:13.4 -- not a known variable star
00:12:54.65 +50:00:36.7 -- not a known variable star
00:13:48.86 +52:27:47.7 -- not a known variable star
00:13:54.18 +55:16:27.8 -- not a known variable star
00:14:00.15 +51:35:37.6 -- a known variable star
00:14:27.07 +56:43:29.1 -- not a known variable star
00:15:10.33 +53:13:09.0 -- not a known variable star
00:19:38.02 +50:48:48.7 -- not a known variable star
00:20:02.57 +50:09:43.6 -- not a known variable star
00:20:03.11 +53:52:00.5 -- not a known variable star
00:20:54.23 +51:47:15.9 -- not a known variable star
00:21:11.81 +54:40:22.6 -- not a known variable star
00:22:41.40 +56:26:52.0 -- not a known variable star
00:22:52.89 +53:18:18.1 -- a known variable star
00:23:20.52 +55:49:18.3 -- not a known variable star
00:23:51.05 +55:31:01.4 -- not a known variable star
00:24:22.17 +53:19:57.7 -- not a known variable star
00:24:22.96 +56:28:07.3 -- a known variable star
00:24:48.07 +53:02:40.7 -- not a known variable star
00:25:09.22 +53:39:27.9 -- not a known variable star
00:25:27.20 +52:39:45.1 -- not a known variable star
00:25:47.94 +52:07:06.0 -- not a known variable star
00:26:15.61 +55:46:37.8 -- not a known variable star
00:27:01.50 +51:15:17.1 -- not a known variable star
00:27:12.05 +54:06:10.9 -- not a known variable star
00:27:40.62 +55:49:21.0 -- not a known variable star
00:28:05.45 +53:55:26.5 -- not a known variable star
00:30:17.74 +55:33:35.7 -- not a known variable star
00:30:27.03 +55:56:11.2 -- not a known variable star
23:10:22.38 +56:52:26.2 -- not a known variable star
23:12:16.25 +55:19:37.7 -- not a known variable star
23:19:50.25 +55:37:38.0 -- not a known variable star
23:20:43.39 +54:46:57.7 -- not a known variable star
23:21:34.07 +55:55:46.4 -- not a known variable star
23:21:42.35 +50:06:37.3 -- not a known variable star
23:22:08.26 +54:51:02.0 -- not a known variable star
23:22:09.42 +54:36:39.8 -- not a known variable star
23:28:24.80 +57:49:21.2 -- not a known variable star
23:28:35.40 +57:13:31.0 -- not a known variable star
23:28:35.99 +50:40:52.8 -- not a known variable star
23:31:39.88 +56:54:31.0 -- not a known variable star
23:33:45.39 +52:44:43.4 -- not a known variable star
23:36:59.18 +56:58:33.6 -- not a known variable star
23:39:40.19 +55:18:36.6 -- not a known variable star
23:50:26.63 +54:13:52.6 -- not a known variable star
23:51:05.94 +53:56:13.3 -- not a known variable star
23:52:27.39 +51:58:26.2 -- not a known variable star
23:55:05.07 +54:12:31.8 -- not a known variable star
23:55:17.18 +50:18:36.8 -- not a known variable star
23:55:26.74 +50:05:20.1 -- not a known variable star
23:56:30.03 +53:45:20.0 -- not a known variable star
23:57:59.98 +50:31:00.1 -- not a known variable star
23:58:01.28 +50:30:16.1 -- not a known variable star
23:58:38.59 +53:55:16.3 -- not a known variable star
23:59:00.94 +53:17:41.6 -- not a known variable star
Found 67 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
74 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 74 (excluding asteroids and hot pixels, 67 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)2461251.87521264 -observatory V36
07:16:27.33 +19:40:36.4 Mercury (0.6mag)
11:30:46.10 +03:16:59.2 Venus (-4.3mag)
05:23:23.51 +23:14:22.7 Mars (1.3mag)
08:34:55.84 +19:10:22.5 Jupiter (-1.8mag)
00:56:48.11 +03:20:23.2 Saturn (0.6mag)
04:10:35.68 +20:53:59.7 Uranus (5.8mag)
00:16:32.75 +00:16:28.7 Neptune (7.7mag)
20:28:59.84 -23:26:38.9 Pluto (14.4mag)
21:12:25.28 -18:04:34.7 Moon (-12.6mag)
-rw-r--r-- 1 apache apache 362 Jul 30 04:24 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461251.87521264:
08:34:58.72 +19:10:10.0 Io (5.9mag)
08:34:49.02 +19:10:51.1 Europa (6.2mag)
08:34:57.02 +19:10:21.6 Ganymede (5.5mag)
08:34:57.61 +19:10:11.9 Callisto (6.7mag)
08:32:41.59 +19:04:30.7 Himalia (15.7mag)
08:34:55.90 +19:10:23.1 Thebe (16.6mag)
08:32:07.79 +19:04:47.5 Elara (17.7mag)
08:38:56.63 +18:54:07.2 Pasiphae (17.9mag)
08:38:41.24 +19:18:49.0 Carme (19.0mag)
00:56:55.10 +03:19:51.4 Titan (8.5mag)
00:56:52.53 +03:20:10.3 Rhea (9.8mag)
00:56:32.56 +03:17:52.8 Iapetus (11.2mag)
00:57:01.42 +03:20:28.7 Hyperion (14.5mag)
00:56:22.10 +03:14:45.5 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 30 04:24 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461251.87521264:
18:30:47.25 -27:01:03.8 JWST
19:08:37.79 +04:58:10.4 Chandra
05:41:32.34 +37:32:03.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 30 04:24 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461251.87521264 -observatory V36
03:03:08.59 +16:35:05.1 17.7mag P/1996 R2 (Lagerkvist)
18:05:08.77 -34:39:03.5 13.9mag P/2010 H2 (Vales)
06:45:24.44 -68:36:04.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:07:19.77 +32:48:46.3 17.7mag C/2017 K2 (PANSTARRS)
03:15:29.94 +32:47:24.5 16.4mag P/2021 N1 (ZTF)
22:45:43.20 +31:53:34.2 17.3mag C/2022 E2 (ATLAS)
06:34:25.72 +26:41:05.9 16.8mag C/2022 N2 (PANSTARRS)
10:13:25.42 +28:52:15.5 16.9mag C/2022 QE78 (ATLAS)
09:22:55.80 +05:15:34.8 17.9mag C/2022 R6 (PANSTARRS)
15:11:22.00 -11:57:36.7 17.8mag P/2023 B1 (PANSTARRS)
21:22:46.92 +66:50:35.8 17.9mag C/2023 H5 (Lemmon)
15:57:59.04 -12:05:46.4 14.2mag C/2023 R1 (PANSTARRS)
07:57:52.70 +30:56:58.2 15.1mag C/2024 E1 (Wierzchos)
15:08:49.00 +15:36:51.1 17.7mag C/2024 G6 (ATLAS)
19:14:40.86 +42:23:25.7 13.7mag C/2024 J3 (ATLAS)
21:23:22.90 +48:30:55.4 17.7mag C/2024 R4 (PANSTARRS)
05:07:47.15 -13:07:03.3 15.5mag C/2024 T5 (ATLAS)
06:50:10.05 +25:41:38.3 17.9mag C/2025 J1 (Borisov)
07:26:38.52 -14:59:16.9 17.4mag C/2025 R3 (PANSTARRS)
10:20:54.06 +21:26:17.1 17.4mag C/2025 V2 (Rankin)
12:53:09.72 +02:54:34.3 17.0mag C/2025 Y1 (ATLAS)
16:09:13.41 +78:33:52.1 17.0mag C/2026 A2 (Bok)
03:03:12.38 +45:58:16.8 17.0mag C/2026 B2 (Sun-Gao)
11:39:42.24 +07:32:02.8 17.2mag A/2026 E1
21:47:48.29 -23:25:40.6 6.9mag 10P/Tempel
11:23:48.68 -02:52:37.5 16.2mag 29P/Schwassmann-Wachmann
04:27:56.26 +31:36:43.0 17.9mag 47P/Ashbrook-Jackson
10:49:34.95 +07:32:16.0 17.2mag 63P/Wild
00:53:59.08 -05:11:18.3 15.5mag 65P/Gunn
05:15:09.61 +20:45:25.5 13.7mag 78P/Gehrels
02:50:59.42 +12:56:51.4 16.6mag 88P/Howell
07:32:37.80 +28:46:30.9 16.0mag 93P/Lovas
03:42:03.08 +13:28:10.2 17.8mag 112P/Urata-Niijima
05:27:05.41 +31:01:53.2 16.4mag 114P/Wiseman-Skiff
08:57:21.27 +28:04:26.6 15.1mag 123P/West-Hartley
11:26:16.16 -06:49:50.7 17.0mag 124P/Mrkos
05:23:14.92 +21:10:11.6 16.1mag 128P/Shoemaker-Holt
06:13:04.20 +19:16:38.8 17.9mag 131P/Mueller
00:04:12.51 +03:25:00.1 17.7mag 139P/Vaisala-Oterma
08:20:12.27 +12:24:06.1 17.9mag 141P-D/Machholz
03:22:19.18 -20:02:45.3 14.4mag 161P/Hartley-IRAS
06:45:06.63 +37:07:53.3 15.7mag 162P/SidingSpring
17:21:26.36 +32:09:55.9 12.9mag 169P/NEAT
02:25:49.10 +09:14:02.7 17.6mag 220P/McNaught
16:37:49.86 -09:28:12.3 17.5mag 235P/LINEAR
20:28:53.26 -52:36:14.6 17.8mag 259P/Garradd
02:56:21.75 +21:19:12.0 15.4mag 260P/McNaught
06:38:27.92 +37:46:21.1 17.3mag 295P/LINEAR
15:08:07.14 +04:05:45.5 17.7mag 391P/Kowalski
08:52:47.80 +18:48:02.8 17.9mag 450P/LONEOS
08:22:34.44 +37:30:36.2 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Jul 30 04:24 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
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
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-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -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
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
-rw-r--r-- 1 apache apache 5.7K Jul 30 04:24 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
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
-rw-r--r-- 1 apache apache 189K Jul 30 04:24 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:56:20.148 +22:48:23.34 AT 2026uez 2026-05-19.43 20.79
17:03:37.940 +40:54:46.91 AT 2026uey 2026-05-17.49 21.43
15:04:21.070 +07:14:23.81 AT 2026uex 2026-06-15.44 20.66
08:49:47.663 -07:24:01.25 AT 2026uew 2026-02-19.37 20.99
04:43:45.409 -21:56:34.12 AT 2026uev 2026-01-14.29 21.36
14:23:02.118 +17:49:57.26 AT 2026ueu 2026-04-20.54 21.18
11:50:55.515 -19:56:24.73 AT 2026uet 2026-01-27.53 21.55
10:59:04.434 -17:05:34.76 AT 2026ues 2026-05-06.27 20.91
15:39:15.006 +12:22:05.73 AT 2026uer 2026-02-13.60 21.8
19:17:04.295 +46:23:18.13 AT 2026ueq 2026-07-01.31 17.5086
08:10:18.850 +45:21:28.27 AT 2026uep 2026-02-21.37 20.88
15:04:40.281 +05:21:56.55 AT 2026ueo 2026-07-09.29 21.15
17:12:49.063 +27:32:51.65 AT 2026uen 2026-07-08.32 19.49
10:28:53.926 +20:07:41.86 AT 2026uem 2026-01-14.45 21.07
11:11:53.428 +13:29:27.96 AT 2026uel 2026-01-29.63 22.38
14:49:01.370 +34:26:52.68 AT 2026uek 2026-06-13.34 20.33
13:48:44.907 -10:17:48.40 AT 2026uej 2026-05-19.33 20.99
14:32:34.192 +18:00:45.73 AT 2026uei 2026-02-13.54 21.3
08:49:51.222 +00:38:50.85 AT 2026ueh 2026-03-09.32 21.51
08:22:39.912 +47:57:53.40 AT 2026ueg 2026-03-06.30 20.74
-rw-r--r-- 1 apache apache 88K Jul 30 04:24 tns_transients_list.txt
