This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q
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 10.1990 2461231.6990 12.20 00:08:25.45 +52:44:49.8
116.35480 -9.57441 galactic Cas Second-epoch detections are separated by 0.5" and 7.3 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 | 00:08:25.45 +52:44:49.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:08:25.45 +52:44:49.8: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:08:25.45 +52:44:49.8: 13.50 +/- 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 10.1990* 00 08 25.45 +52 44 49.8 12.2 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,2461231.6990,12.20,0.05,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 20260710.1990 12.20CV 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 10.1990 2461231.6990 12.10 00:17:49.50 +53:38:52.4
117.90190 -8.89526 galactic Cas Second-epoch detections are separated by 3.0" 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 | 00:17:49.50 +53:38:52.4 (user input) | T | P | (position from user input) J-Ks=0.485+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:49.50 +53:38:52.4: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:49.50 +53:38:52.4: 13.54 +/- 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 10.1990* 00 17 49.50 +53 38 52.4 12.1 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,2461231.6990,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1990 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.97 00:13:43.57 +53:21:57.3
117.25108 -9.08936 galactic Cas Second-epoch detections are separated by 1.2" and 7.3 pix
The object was found in VSX16" Gaia DR3 419997984230979968
Type: VAR
# Max. Min./Amp. JD0 Period
13.130 G 13.200 G 0.014385200000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:13:43.57 +53:21:57.3: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:13:43.57 +53:21:57.3: 13.54 +/- 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 10.1990* 00 13 43.57 +53 21 57.3 12.0 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 419997984230979968,2461231.6990,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419997984230979968 20260710.1990 11.97CV 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 10.1990 2461231.6990 11.96 23:44:27.37 +49:42:04.3
111.95994 -11.73824 galactic Cas Second-epoch detections are separated by 3.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.1125+49.6989 | 23:44:27.37 +49:42:04.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.279+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:44:27.37 +49:42:04.3: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:44:27.37 +49:42:04.3: 13.60 +/- 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 10.1990* 23 44 27.37 +49 42 04.3 12.0 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 J356.1125+49.6989,2461231.6990,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.1125+49.6989 20260710.1990 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.80 00:15:45.53 +53:37:27.3
117.59153 -8.87713 galactic Cas Second-epoch detections are separated by 1.6" and 7.2 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 | 00:15:45.53 +53:37:27.3 (user input) | T | P | (position from user input) J-Ks=0.973+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:15:45.53 +53:37:27.3: 13.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:15:45.53 +53:37:27.3: 13.57 +/- 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 10.1990* 00 15 45.53 +53 37 27.3 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
target,2461231.6990,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1990 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.78 00:22:00.94 +54:12:53.0
118.59180 -8.40890 galactic Cas Second-epoch detections are separated by 2.6" 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 | Gaia DR3 419723656079834624 | 00:21:59.08 +54:13:07.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.347+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:22:00.94 +54:12:53.0: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:22:00.94 +54:12:53.0: 13.50 +/- 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 10.1990* 00 22 00.94 +54 12 53.0 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 419723656079834624,2461231.6990,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419723656079834624 20260710.1990 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.52 00:26:37.85 +53:22:52.5
119.18791 -9.31007 galactic Cas Second-epoch detections are separated by 1.4" 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 | ATO J006.6517+53.3880 | 00:26:37.85 +53:22:52.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.291+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:26:37.85 +53:22:52.5: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:37.85 +53:22:52.5: 13.45 +/- 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 10.1990* 00 26 37.85 +53 22 52.5 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 J006.6517+53.3880,2461231.6990,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.6517+53.3880 20260710.1990 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.71 23:45:04.91 +50:54:58.8
112.38053 -10.59095 galactic Cas Second-epoch detections are separated by 2.9" and 6.9 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 | 23:45:04.91 +50:54:58.8 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:45:04.91 +50:54:58.8: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:45:04.91 +50:54:58.8: 13.54 +/- 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 10.1990* 23 45 04.91 +50 54 58.8 11.7 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,2461231.6990,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1990 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.72 00:24:54.44 +53:26:45.2
118.93562 -9.21987 galactic Cas Second-epoch detections are separated by 2.2" 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 419472344650653312 | 00:24:52.91 +53:26:31.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.351+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:24:54.44 +53:26:45.2: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:24:54.44 +53:26:45.2: 13.48 +/- 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 10.1990* 00 24 54.44 +53 26 45.2 11.7 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 419472344650653312,2461231.6990,11.72,0.05,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
Gaia DR3 419472344650653312 20260710.1990 11.72CV 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 10.1990 2461231.6990 11.76 00:07:18.07 +57:21:29.2
116.98365 -5.00301 galactic Cas Second-epoch detections are separated by 2.0" and 7.0 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 J001.8287+57.3578 | 00:07:18.07 +57:21:29.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:18.07 +57:21:29.2: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:18.07 +57:21:29.2: 13.52 +/- 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 10.1990* 00 07 18.07 +57 21 29.2 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
ATO J001.8287+57.3578,2461231.6990,11.76,0.05,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 J001.8287+57.3578 20260710.1990 11.76CV 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 10.1990 2461231.6990 11.68 00:31:11.15 +56:36:29.2
120.13180 -6.15349 galactic Cas Second-epoch detections are separated by 1.3" and 7.6 pix
The object was found in VSX 1" ZTF J003111.04+563629.4
Type: RS
# Max. Min./Amp. JD0 Period
13.678 g Y 0.049 g 2458292.94960 2.269195400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:11.15 +56:36:29.2: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:11.15 +56:36:29.2: 13.42 +/- 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 10.1990* 00 31 11.15 +56 36 29.2 11.7 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
ZTF J003111.04+563629.4,2461231.6990,11.68,0.05,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 J003111.04+563629.4 20260710.1990 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.64 23:49:13.51 +52:28:15.9
113.40642 -9.24626 galactic Cas Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1945286384531274880 | 23:49:14.01 +52:27:56.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.827+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:49:13.51 +52:28:15.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:49:13.51 +52:28:15.9: 13.50 +/- 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 10.1990* 23 49 13.51 +52 28 15.9 11.6 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 1945286384531274880,2461231.6990,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1945286384531274880 20260710.1990 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.69 23:54:13.46 +50:19:54.5
113.67035 -11.50826 galactic Cas Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1940987981263609216 | 23:54:11.41 +50:19:56.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.425+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:13.46 +50:19:54.5: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:54:13.46 +50:19:54.5: 13.54 +/- 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 10.1990* 23 54 13.46 +50 19 54.5 11.7 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 1940987981263609216,2461231.6990,11.69,0.05,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 1940987981263609216 20260710.1990 11.69CV 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 10.1990 2461231.6990 11.53 00:11:44.31 +50:55:16.2
116.56694 -11.45930 galactic Cas Second-epoch detections are separated by 1.2" and 7.3 pix
The object was found in VSX20" Gaia DR3 395358306610419456
Type: RS
# Max. Min./Amp. JD0 Period
11.860 G 12.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:11:44.31 +50:55:16.2: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:11:44.31 +50:55:16.2: 13.57 +/- 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 10.1990* 00 11 44.31 +50 55 16.2 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
Gaia DR3 395358306610419456,2461231.6990,11.53,0.05,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 395358306610419456 20260710.1990 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.55 23:52:02.79 +55:16:14.3
114.48063 -6.62357 galactic Cas Second-epoch detections are separated by 1.9" and 7.2 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 | 23:52:02.79 +55:16:14.3 (user input) | T | P | (position from user input) J-Ks=0.293+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:52:02.79 +55:16:14.3: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:52:02.79 +55:16:14.3: 13.55 +/- 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 10.1990* 23 52 02.79 +55 16 14.3 11.6 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,2461231.6990,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1990 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.39 00:27:05.56 +53:23:17.9
119.25806 -9.30969 galactic Cas Second-epoch detections are separated by 1.0" 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 | Gaia DR3 419427234618930944 | 00:27:02.46 +53:23:21.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.771+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:05.56 +53:23:17.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:05.56 +53:23:17.9: 13.46 +/- 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 10.1990* 00 27 05.56 +53 23 17.9 11.4 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 419427234618930944,2461231.6990,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419427234618930944 20260710.1990 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.57 00:29:10.98 +56:03:03.6
119.80692 -6.68566 galactic Cas Second-epoch detections are separated by 1.6" and 7.3 pix
The object was found in VSX 6" Gaia DR3 421291903258832896
Type: S
# Max. Min./Amp. JD0 Period
14.050 G 14.390 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:10.98 +56:03:03.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:10.98 +56:03:03.6: 13.45 +/- 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 10.1990* 00 29 10.98 +56 03 03.6 11.6 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 421291903258832896,2461231.6990,11.57,0.05,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 421291903258832896 20260710.1990 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.1990 2461231.6990 11.36 00:25:59.34 +52:05:26.3
118.96019 -10.58475 galactic Cas Second-epoch detections are separated by 2.3" 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 | Gaia DR3 418897441808300416 | 00:26:01.38 +52:05:38.1 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.640+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:59.34 +52:05:26.3: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:59.34 +52:05:26.3: 13.49 +/- 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 10.1990* 00 25 59.34 +52 05 26.3 11.4 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 418897441808300416,2461231.6990,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 418897441808300416 20260710.1990 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.48 23:40:34.07 +56:55:03.6
113.33841 -4.62820 galactic Cas Second-epoch detections are separated by 4.2" and 7.0 pix
The object was found in VSX18" Gaia DR3 1997892655805203840
Type: ROT
# Max. Min./Amp. JD0 Period
14.140 G 14.170 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:40:34.07 +56:55:03.6: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:40:34.07 +56:55:03.6: 13.55 +/- 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 10.1990* 23 40 34.07 +56 55 03.6 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
Gaia DR3 1997892655805203840,2461231.6990,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997892655805203840 20260710.1990 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.26 23:48:06.79 +50:03:10.1
112.63312 -11.54841 galactic Cas Second-epoch detections are separated by 4.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1943874680320287232 | 23:48:08.46 +50:03:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.360+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:48:06.79 +50:03:10.1: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:48:06.79 +50:03:10.1: 13.49 +/- 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 10.1990* 23 48 06.79 +50 03 10.1 11.3 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 1943874680320287232,2461231.6990,11.26,0.05,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
Gaia DR3 1943874680320287232 20260710.1990 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.21 23:36:06.87 +52:01:25.7
111.32651 -9.14254 galactic Cas Second-epoch detections are separated by 0.5" and 6.8 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 | ATO J354.0454+52.0178 | 23:36:08.75 +52:01:07.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.361+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:36:06.87 +52:01:25.7: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:36:06.87 +52:01:25.7: 13.58 +/- 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 10.1990* 23 36 06.87 +52 01 25.7 11.2 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 J354.0454+52.0178,2461231.6990,11.21,0.05,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
ATO J354.0454+52.0178 20260710.1990 11.21CV 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 10.1990 2461231.6990 11.31 23:59:28.49 +55:55:50.2
115.65465 -6.20519 galactic Cas Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1994723244817931392 | 23:59:28.12 +55:56:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.736+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:28.49 +55:55:50.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:28.49 +55:55:50.2: 13.38 +/- 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 10.1990* 23 59 28.49 +55 55 50.2 11.3 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 1994723244817931392,2461231.6990,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994723244817931392 20260710.1990 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.15 00:23:06.53 +53:52:58.8
118.71508 -8.75664 galactic Cas Second-epoch detections are separated by 2.3" and 7.5 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 | ZTF DR3 | 00:23:06.39 +53:52:37.5 (Gaia DR3) | 773107400040014 (VSX @ VizieR) | RR: (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.407+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:23:06.53 +53:52:58.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:06.53 +53:52:58.8: 13.49 +/- 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 10.1990* 00 23 06.53 +53 52 58.8 11.2 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 DR3,2461231.6990,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF DR3 20260710.1990 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.24 23:57:24.25 +51:41:40.7
114.46977 -10.28712 galactic Cas Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1944137016924801920 | 23:57:26.96 +51:41:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.062+/-0.040 (A)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:24.25 +51:41:40.7: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:24.25 +51:41:40.7: 13.54 +/- 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 10.1990* 23 57 24.25 +51 41 40.7 11.2 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 1944137016924801920,2461231.6990,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944137016924801920 20260710.1990 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.19 23:54:58.16 +50:29:55.1
113.82634 -11.37208 galactic Cas Second-epoch detections are separated by 0.5" and 7.2 pix
The object was found in VSX15" Gaia DR3 1941007463235207808
Type: ROT
# Max. Min./Amp. JD0 Period
12.990 G 13.070 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:58.16 +50:29:55.1: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:54:58.16 +50:29:55.1: 13.56 +/- 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 10.1990* 23 54 58.16 +50 29 55.1 11.2 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 1941007463235207808,2461231.6990,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1941007463235207808 20260710.1990 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.00 00:30:23.79 +55:49:09.7
119.95772 -6.93083 galactic Cas Second-epoch detections are separated by 2.3" and 7.5 pix
The object was found in VSX17" Gaia DR3 421273280280788608
Type: ROT
# Max. Min./Amp. JD0 Period
15.310 G 15.340 G G
ATTENTION: measured mag 11.00 is 4.3 mag brighter than the VSX record maximum brightness 15.31 - 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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:23.79 +55:49:09.7: 13.45 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:23.79 +55:49:09.7: 13.45 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.45 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 10.1990* 00 30 23.79 +55 49 09.7 11.0 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 421273280280788608,2461231.6990,11.00,0.05,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 421273280280788608 20260710.1990 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.22 23:53:38.29 +51:20:56.6
113.81180 -10.49629 galactic Cas Second-epoch detections are separated by 3.7" 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 J358.4052+51.3477 | 23:53:40.47 +51:20:39.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:53:38.29 +51:20:56.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:53:38.29 +51:20:56.6: 13.59 +/- 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 10.1990* 23 53 38.29 +51 20 56.6 11.2 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 J358.4052+51.3477,2461231.6990,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.4052+51.3477 20260710.1990 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.19 00:03:55.02 +55:04:36.7
116.11015 -7.16423 galactic Cas Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J000.9974+55.0797 | 00:03:55.02 +55:04:36.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.296+/-0.032 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:03:55.02 +55:04:36.7: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:03:55.02 +55:04:36.7: 13.58 +/- 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 10.1990* 00 03 55.02 +55 04 36.7 11.2 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 J000.9974+55.0797,2461231.6990,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J000.9974+55.0797 20260710.1990 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.04 00:28:47.80 +56:39:17.4
119.80649 -6.07946 galactic Cas Second-epoch detections are separated by 1.3" and 7.3 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 J007.1958+56.6564 | 00:28:47.80 +56:39:17.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.208+/-0.031 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:47.80 +56:39:17.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:47.80 +56:39:17.4: 13.33 +/- 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 10.1990* 00 28 47.80 +56 39 17.4 11.0 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 J007.1958+56.6564,2461231.6990,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J007.1958+56.6564 20260710.1990 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 10.96 00:01:22.29 +51:04:01.3
114.95623 -11.02775 galactic Cas Second-epoch detections are separated by 2.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 394059233623834112 | 00:01:26.54 +51:03:56.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.414+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:01:22.29 +51:04:01.3: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:01:22.29 +51:04:01.3: 13.50 +/- 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 10.1990* 00 01 22.29 +51 04 01.3 11.0 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 394059233623834112,2461231.6990,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 394059233623834112 20260710.1990 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.27 23:29:04.49 +50:59:57.2
109.95271 -9.78513 galactic Cas Second-epoch detections are separated by 2.0" and 7.1 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 J352.2776+50.9956 | 23:29:04.49 +50:59:57.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:04.49 +50:59:57.2: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:04.49 +50:59:57.2: 13.54 +/- 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 10.1990* 23 29 04.49 +50 59 57.2 11.3 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
ATO J352.2776+50.9956,2461231.6990,11.27,0.05,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
ATO J352.2776+50.9956 20260710.1990 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.16 23:58:11.84 +50:30:00.0
114.33806 -11.48124 galactic Cas Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1940966472068395008 | 23:58:14.42 +50:29:39.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:11.84 +50:30:00.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:11.84 +50:30:00.0: 13.38 +/- 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 10.1990* 23 58 11.84 +50 30 00.0 11.2 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 1940966472068395008,2461231.6990,11.16,0.05,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
Gaia DR3 1940966472068395008 20260710.1990 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.09 23:19:23.42 +54:59:23.2
109.90948 -5.53770 galactic Cas Second-epoch detections are separated by 0.5" and 6.6 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 1996825712907076608 | 23:19:23.65 +54:59:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.313+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:19:23.42 +54:59:23.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:19:23.42 +54:59:23.2: 13.48 +/- 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 10.1990* 23 19 23.42 +54 59 23.2 11.1 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
Gaia DR3 1996825712907076608,2461231.6990,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996825712907076608 20260710.1990 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.23 23:20:19.19 +56:57:19.9
110.71701 -3.73957 galactic Cas Second-epoch detections are separated by 2.3" and 6.7 pix
The object was found in VSX17" Gaia DR3 2009328470082840960
Type: E
# Max. Min./Amp. JD0 Period
12.320 G 12.350 G 1.487580000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:20:19.19 +56:57:19.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:20:19.19 +56:57:19.9: 13.31 +/- 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 10.1990* 23 20 19.19 +56 57 19.9 11.2 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 2009328470082840960,2461231.6990,11.23,0.05,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
Gaia DR3 2009328470082840960 20260710.1990 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 10.92 23:46:36.49 +51:42:15.2
112.81931 -9.89008 galactic Cas Second-epoch detections are separated by 1.2" and 6.8 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 1945016110828646912 | 23:46:35.08 +51:42:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.706+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:46:36.49 +51:42:15.2: 13.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:36.49 +51:42:15.2: 13.62 +/- 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 10.1990* 23 46 36.49 +51 42 15.2 10.9 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
Gaia DR3 1945016110828646912,2461231.6990,10.92,0.05,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
Gaia DR3 1945016110828646912 20260710.1990 10.92CV 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 10.1990 2461231.6990 10.81 00:29:03.26 +55:22:32.7
119.72941 -7.35675 galactic Cas Second-epoch detections are separated by 2.9" and 7.5 pix
The object was found in VSX16" ZTF J002905.03+552227.5
Type: EW
# Max. Min./Amp. JD0 Period
17.943 g Y 0.388 g 2458307.90690 0.360202000000
ATTENTION: measured mag 10.81 is 6.7 mag brighter than the VSX record maximum brightness 17.55 - 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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:03.26 +55:22:32.7: 13.14 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:03.26 +55:22:32.7: 12.66 +/- 0.18 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 10.1990* 00 29 03.26 +55 22 32.7 10.8 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
ZTF J002905.03+552227.5,2461231.6990,10.81,0.05,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 J002905.03+552227.5 20260710.1990 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.1990 2461231.6990 10.81 00:28:46.33 +54:50:14.8
119.64100 -7.88941 galactic Cas Second-epoch detections are separated by 1.7" and 7.8 pix
The object was found in VSX 2" Gaia DR3 421103298351769728
Type: ROT
# Max. Min./Amp. JD0 Period
12.550 G 12.580 G 1.755940000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:46.33 +54:50:14.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:46.33 +54:50:14.8: 13.38 +/- 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 10.1990* 00 28 46.33 +54 50 14.8 10.8 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 421103298351769728,2461231.6990,10.81,0.05,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 421103298351769728 20260710.1990 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 10.1990 2461231.6990 10.52 23:57:09.56 +50:24:07.3
114.15213 -11.54213 galactic Cas Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1940965132036769408 | 23:57:07.17 +50:23:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.815+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:09.56 +50:24:07.3: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:09.56 +50:24:07.3: 13.43 +/- 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 10.1990* 23 57 09.56 +50 24 07.3 10.5 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
Gaia DR3 1940965132036769408,2461231.6990,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940965132036769408 20260710.1990 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 10.22 00:28:10.83 +56:29:43.0
119.70712 -6.23078 galactic Cas Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421682195525573504 | 00:28:13.11 +56:30:07.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:10.83 +56:29:43.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:10.83 +56:29:43.0: 13.41 +/- 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 10.1990* 00 28 10.83 +56 29 43.0 10.2 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 421682195525573504,2461231.6990,10.22,0.05,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 421682195525573504 20260710.1990 10.22CV 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 10.1990 2461231.6990 10.04 00:15:03.76 +51:59:23.5
117.25151 -10.48024 galactic Cas Second-epoch detections are separated by 1.9" and 7.5 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 | ATO J003.7488+51.9921 | 00:15:02.21 +51:59:36.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.227+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:15:03.76 +51:59:23.5: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:15:03.76 +51:59:23.5: 13.56 +/- 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 10.1990* 00 15 03.76 +51 59 23.5 10.0 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 J003.7488+51.9921,2461231.6990,10.04,0.05,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
ATO J003.7488+51.9921 20260710.1990 10.04CV 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 10.1990 2461231.6990 10.39 00:14:07.39 +51:33:28.3
117.04144 -10.88661 galactic Cas Second-epoch detections are separated by 0.7" and 7.3 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 | ASASSN-V J001410.11+513334.1 | 00:14:10.11 +51:33:34.1 (Gaia DR3) | SR (local) | 144.000000000000 (local) | Gaia3var=VARIABLE SpType: MS 1984PW&SO...3....1S CSS 5 J-Ks=0.345+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:14:07.39 +51:33:28.3: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:14:07.39 +51:33:28.3: 13.46 +/- 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 10.1990* 00 14 07.39 +51 33 28.3 10.4 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
ASASSN-V J001410.11+513334.1,2461231.6990,10.39,0.05,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
ASASSN-V J001410.11+513334.1 20260710.1990 10.39CV 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 10.1990 2461231.6990 10.39 00:28:42.04 +57:00:50.5
119.82527 -5.72051 galactic Cas Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX23" Gaia DR3 421813484080843904
Type: E
# Max. Min./Amp. JD0 Period
10.900 G 10.960 G 3.371510000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:42.04 +57:00:50.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:42.04 +57:00:50.5: 13.37 +/- 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 10.1990* 00 28 42.04 +57 00 50.5 10.4 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 421813484080843904,2461231.6990,10.39,0.05,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 421813484080843904 20260710.1990 10.39CV 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 10.1990 2461231.6990 10.66 00:25:23.89 +55:26:50.9
119.21548 -7.23626 galactic Cas Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421200575075768832 | 00:25:26.59 +55:26:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.645+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:23.89 +55:26:50.9: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:23.89 +55:26:50.9: 13.45 +/- 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 10.1990* 00 25 23.89 +55 26 50.9 10.7 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 421200575075768832,2461231.6990,10.66,0.05,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
Gaia DR3 421200575075768832 20260710.1990 10.66CV 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 10.1990 2461231.6990 11.07 00:19:32.87 +57:40:50.6
118.66356 -4.92650 galactic Cas Second-epoch detections are separated by 2.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 422040911198672384 | 00:19:36.72 +57:40:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.229+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:32.87 +57:40:50.6: 13.53 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:32.87 +57:40:50.6: 13.31 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.53 +/- 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 10.1990* 00 19 32.87 +57 40 50.6 11.1 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
Gaia DR3 422040911198672384,2461231.6990,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 422040911198672384 20260710.1990 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.14 00:20:17.97 +57:39:09.9
118.76024 -4.96656 galactic Cas Second-epoch detections are separated by 1.4" and 7.3 pix
The object was found in VSX25" Gaia DR3 422045755920643968
Type: ROT
# Max. Min./Amp. JD0 Period
16.740 G 16.810 G K
ATTENTION: measured mag 11.14 is 5.6 mag brighter than the VSX record maximum brightness 16.74 - 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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:20:17.97 +57:39:09.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:20:17.97 +57:39:09.9: 13.49 +/- 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 10.1990* 00 20 17.97 +57 39 09.9 11.1 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
Gaia DR3 422045755920643968,2461231.6990,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 422045755920643968 20260710.1990 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.22 00:04:13.50 +51:32:55.6
115.49555 -10.63999 galactic Cas Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 395541237856954880 | 00:04:16.83 +51:32:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:04:13.50 +51:32:55.6: 13.29 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:04:13.50 +51:32:55.6: 13.43 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 10.1990* 00 04 13.50 +51 32 55.6 11.2 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 395541237856954880,2461231.6990,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 395541237856954880 20260710.1990 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.45 00:06:29.46 +50:07:48.1
115.59204 -12.10007 galactic Cas Second-epoch detections are separated by 2.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.6233+50.1303 | 00:06:26.54 +50:07:38.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.156+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:06:29.46 +50:07:48.1: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:06:29.46 +50:07:48.1: 13.53 +/- 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 10.1990* 00 06 29.46 +50 07 48.1 11.4 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 J001.6233+50.1303,2461231.6990,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.6233+50.1303 20260710.1990 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.71 00:00:49.22 +49:57:54.5
114.64594 -12.09050 galactic Cas Second-epoch detections are separated by 5.4" and 6.9 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 393887434931742720 | 00:00:46.95 +49:58:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.531+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:00:49.22 +49:57:54.5: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:00:49.22 +49:57:54.5: 13.54 +/- 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 10.1990* 00 00 49.22 +49 57 54.5 11.7 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 393887434931742720,2461231.6990,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 393887434931742720 20260710.1990 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.64 00:21:04.97 +51:45:18.7
118.15748 -10.83493 galactic Cas Second-epoch detections are separated by 3.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 394899982055064192 | 00:21:06.67 +51:45:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.507+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:21:04.97 +51:45:18.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:21:04.97 +51:45:18.7: 13.38 +/- 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 10.1990* 00 21 04.97 +51 45 18.7 11.6 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 394899982055064192,2461231.6990,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 394899982055064192 20260710.1990 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1990 2461231.6990 11.96 00:00:56.14 +53:53:48.0
115.45426 -8.24024 galactic Cas Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 396303714812067200 | 00:00:52.93 +53:54:04.6 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE SpType: G8 (LAMOST DR5) J-Ks=0.681+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:00:56.14 +53:53:48.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:00:56.14 +53:53:48.0: 13.46 +/- 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 10.1990* 00 00 56.14 +53 53 48.0 12.0 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 396303714812067200,2461231.6990,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 396303714812067200 20260710.1990 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
First image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461231.69944381 10.07.2026 04:47:01.945 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.79
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17127
Objects passed selection criteria: 17083
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: 13533.5
Average stars matched: 13206.8 (97.5856 %)
Memory usage VmPeak: 123488 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 03:53:02 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: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
First image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461231.69944381 10.07.2026 04:47:01.945 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 127
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 281 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 132861
Objects passed selection criteria: 132547
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 111190
Average stars matched: 107784 (96.9366 %)
Memory usage VmPeak: 1967860 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 04:02:11 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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: 2461231.69853844
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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Image size: 927.0'x616.4' 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: 00:00:01.466 +54:00:23.28 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:04.584 +54:00:28.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 00:00:04.584 +54:00:28.17
Angular distance between the image centers 0.0078 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
Image size: 939.0'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:04.235 +53:59:45.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 00:00:04.235 +53:59:45.29
Angular distance between the image centers 0.0125 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 00:00:04.584 +54:00:28.17
Second-epoch second image center 00:00:04.235 +53:59:45.29
Angular distance between the image centers 0.01194 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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits &> /tmp/tmp.zxxWXU57tj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits &> /tmp/tmp.RtTNJCLZFq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits &> /tmp/tmp.VzuEga701F
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits &> /tmp/tmp.wUGS89Wd9y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 23386 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0031 to 359.9999 deg, Dec +48.2162 to +59.2586 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 0.0031 to 359.9999 deg, Dec 48.2162 to 59.2586 deg
Loaded 153985 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): 53 out of 58 total matches.
Matched with Tycho-2 58 out of 23386 detected stars.
ERROR: only 53 of 23386 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.23%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.473500
a=0.000000 b=1.000000 c=22.473500
From vast_summary.log: estimated ref. image limiting mag.: -7.79
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.68
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23386 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0031 to 359.9999 deg, Dec +48.2162 to +59.2586 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 0.0031 to 359.9999 deg, Dec 48.2162 to 59.2586 deg
Loaded 153985 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): 53 out of 58 total matches.
Matched with Tycho-2 58 out of 23386 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (aperture=6.2)
Read 23366 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0031 to 360.0000 deg, Dec +48.2161 to +59.2689 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 0.0031 to 360.0000 deg, Dec 48.2161 to 59.2689 deg
Loaded 154106 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): 50 out of 55 total matches.
Matched with Tycho-2 55 out of 23366 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
2.5 pix fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
2.4 pix fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
2.3 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Limiting magnitude estimates:
14.7 mag. Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
14.7 mag. Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
13.8 mag. fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
13.8 mag. fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zxxWXU57tj (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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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=1910, bad_region=5051, passed=23386
Got 23386 stars (including 16726 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 23386 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.0'
Seting catalog search parameters based on the expected field of view 927.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012875 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010300 (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 344.9996 through 0 to 14.8812, gap 14.8812 to 344.9996
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 325 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 241 matched stars entering correct_measured_positions(), 168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 4908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.09"
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 344.9814 through 0 to 14.9033, gap 14.9033 to 344.9814
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 397 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 328 matched stars entering correct_measured_positions(), 4961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.99"
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 6645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.24"
Excluding outliers - 325 stars left (next iteration limit 256)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits N_match=325 sigma_overall_arcsec=11.131 sigma_q1_arcsec=25.602 sigma_q2_arcsec=32.104 sigma_q3_arcsec=8.250 sigma_q4_arcsec=9.745 n_q1=41 n_q2=23 n_q3=116 n_q4=145 worst_quadrant_to_overall_ratio=2.884
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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.RtTNJCLZFq (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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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=1872, bad_region=4985, passed=23366
Got 23366 stars (including 16797 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 23366 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.1'
Seting catalog search parameters based on the expected field of view 927.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012876 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010301 (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 345.0112 through 0 to 14.8810, gap 14.8810 to 345.0112
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 239 matched stars entering correct_measured_positions(), 165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 231 matched stars entering correct_measured_positions(), 4693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.88"
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 344.9936 through 0 to 14.9023, gap 14.9023 to 344.9936
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 397 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 321 matched stars entering correct_measured_positions(), 4741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.79"
Accuracy estimation diagnostic: 315 matched stars entering correct_measured_positions(), 6313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.43"
Excluding outliers - 315 stars left (next iteration limit 254)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits N_match=315 sigma_overall_arcsec=10.449 sigma_q1_arcsec=28.329 sigma_q2_arcsec=30.359 sigma_q3_arcsec=8.438 sigma_q4_arcsec=7.803 n_q1=34 n_q2=19 n_q3=120 n_q4=142 worst_quadrant_to_overall_ratio=2.905
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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.VzuEga701F (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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.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_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.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=653, bad_region=1808, passed=10522
Got 10522 stars (including 8164 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat
util/solve_plate_with_UCAC5 got 10522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 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 344.8507 through 0 to 14.6555, gap 14.6555 to 344.8507
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 8853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 344.8488 through 0 to 14.6563, gap 14.6563 to 344.8488
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 8854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 8854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits N_match=969 sigma_overall_arcsec=0.622 sigma_q1_arcsec=0.663 sigma_q2_arcsec=0.595 sigma_q3_arcsec=0.679 sigma_q4_arcsec=0.511 n_q1=303 n_q2=143 n_q3=332 n_q4=191 worst_quadrant_to_overall_ratio=1.092
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.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.wUGS89Wd9y (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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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=721, bad_region=1921, passed=10933
Got 10933 stars (including 8409 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat
util/solve_plate_with_UCAC5 got 10933 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 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 344.8504 through 0 to 14.6558, gap 14.6558 to 344.8504
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 9170 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 344.8486 through 0 to 14.6566, gap 14.6566 to 344.8486
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 9169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 9169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits N_match=970 sigma_overall_arcsec=0.695 sigma_q1_arcsec=0.694 sigma_q2_arcsec=0.652 sigma_q3_arcsec=0.770 sigma_q4_arcsec=0.556 n_q1=316 n_q2=149 n_q3=324 n_q4=181 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits sigma_overall=11.131 worst_q_ratio=2.884
ref2=Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits sigma_overall=10.449 worst_q_ratio=2.905
new1=fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits sigma_overall=0.622 worst_q_ratio=1.092
new2=fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits sigma_overall=0.695 worst_q_ratio=1.107
reference average sigma_overall=10.79 worst_q_ratio=2.8945
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006_astrometric_residuals.png (325 matched stars from wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.67 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007_astrometric_residuals.png (315 matched stars from wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.55 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124_astrometric_residuals.png (969 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.55 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125_astrometric_residuals.png (970 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.62 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:11:31.29 +56:01:29.1: 14.89 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:11:31.29 +56:01:29.1: 14.71 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.19
Forced photometry filter KEPT candidate at 23:11:31.29 +56:01:29.1: ref_mag=14.79 +/- 0.19 new_mean_mag=11.2414 delta=3.54 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out31286.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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 31235_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 31235_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:54:23.18 +53:19:21.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31286_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 31286_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:11:31.29 +56:01:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 2.420 2008809775475447808 347.87925297910 +56.02499225483 10.8688 9.6810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17508_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 17508_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:44:32.03 +56:34:49.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05724_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 05724_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:09:36.57 +51:34:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14592_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 14592_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:04:40.69 +55:32:14.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
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 ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Image size: 927.0'x616.4' 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: 00:00:01.466 +54:00:23.28 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:04.584 +54:00:28.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 00:00:04.584 +54:00:28.17
Angular distance between the image centers 0.0078 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
Image size: 939.0'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:04.235 +53:59:45.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 00:00:04.235 +53:59:45.29
Angular distance between the image centers 0.0125 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 00:00:04.584 +54:00:28.17
Second-epoch second image center 00:00:04.235 +53:59:45.29
Angular distance between the image centers 0.01194 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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits &> /tmp/tmp.NOz9hMIU69
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits &> /tmp/tmp.aWhwKS4pvG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits &> /tmp/tmp.VvAb9vvyNm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits &> /tmp/tmp.xMMFLgz9DE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 167282 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +48.1859 to +59.2631 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 0.0000 to 360.0000 deg, Dec 48.1859 to 59.2631 deg
Loaded 154477 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): 105 out of 150 total matches.
Matched with Tycho-2 150 out of 167282 detected stars.
ERROR: only 105 of 167282 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.06%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.702700
a=0.000000 b=1.000000 c=20.702700
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 167282 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +48.1859 to +59.2631 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 0.0000 to 360.0000 deg, Dec 48.1859 to 59.2631 deg
Loaded 154477 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): 105 out of 150 total matches.
Matched with Tycho-2 150 out of 167282 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (aperture=4.7)
Read 165704 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +48.1861 to +59.2705 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 0.0000 to 360.0000 deg, Dec 48.1861 to 59.2705 deg
Loaded 154563 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): 102 out of 145 total matches.
Matched with Tycho-2 145 out of 165704 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 97 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.2 pix Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
2.1 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Limiting magnitude estimates:
13.3 mag. Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
13.2 mag. Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
12.3 mag. fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
12.4 mag. fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
All-image limiting magnitude estimate: 12.3 (SNR ) 11.8 (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.NOz9hMIU69 (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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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=35, blended=20826, bad_region=21165, passed=167247
Got 167247 stars (including 127895 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 167247 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.0'
Seting catalog search parameters based on the expected field of view 927.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012875 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010300 (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 344.9631 through 0 to 14.9764, gap 14.9764 to 344.9631
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 318 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 216 matched stars entering correct_measured_positions(), 35553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.38"
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 344.9503 through 0 to 14.9983, gap 14.9983 to 344.9503
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 395 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 320 matched stars entering correct_measured_positions(), 35597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.35"
Accuracy estimation diagnostic: 315 matched stars entering correct_measured_positions(), 52070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.79"
Excluding outliers - 315 stars left (next iteration limit 237)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits N_match=315 sigma_overall_arcsec=8.955 sigma_q1_arcsec=30.923 sigma_q2_arcsec=19.444 sigma_q3_arcsec=6.520 sigma_q4_arcsec=8.008 n_q1=39 n_q2=21 n_q3=117 n_q4=138 worst_quadrant_to_overall_ratio=3.453
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.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.aWhwKS4pvG (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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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=39, blended=20515, bad_region=20705, passed=165665
Got 165665 stars (including 126839 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 165665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.1'
Seting catalog search parameters based on the expected field of view 927.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012876 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010301 (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 344.9474 through 0 to 14.9341, gap 14.9341 to 344.9474
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 326 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 225 matched stars entering correct_measured_positions(), 37244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.65"
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 344.9404 through 0 to 14.9637, gap 14.9637 to 344.9404
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 400 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 37289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.64"
Accuracy estimation diagnostic: 317 matched stars entering correct_measured_positions(), 52373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.41"
Excluding outliers - 317 stars left (next iteration limit 247)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits N_match=317 sigma_overall_arcsec=8.596 sigma_q1_arcsec=27.471 sigma_q2_arcsec=23.969 sigma_q3_arcsec=6.420 sigma_q4_arcsec=8.419 n_q1=37 n_q2=20 n_q3=128 n_q4=132 worst_quadrant_to_overall_ratio=3.196
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.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.VvAb9vvyNm (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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.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_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.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=21, blended=7100, bad_region=14719, passed=90960
Got 90960 stars (including 69848 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat
util/solve_plate_with_UCAC5 got 90960 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 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 344.8123 through 0 to 14.8108, gap 14.8108 to 344.8123
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 78107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 344.8105 through 0 to 14.8119, gap 14.8119 to 344.8105
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 78107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 78107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits N_match=973 sigma_overall_arcsec=0.588 sigma_q1_arcsec=0.612 sigma_q2_arcsec=0.563 sigma_q3_arcsec=0.657 sigma_q4_arcsec=0.535 n_q1=326 n_q2=159 n_q3=290 n_q4=198 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.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.xMMFLgz9DE (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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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=7792, bad_region=15522, passed=95640
Got 95640 stars (including 73027 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat
util/solve_plate_with_UCAC5 got 95640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 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 344.8109 through 0 to 14.8108, gap 14.8108 to 344.8109
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 82282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 344.8092 through 0 to 14.8117, gap 14.8117 to 344.8092
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 82282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 82281 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 975 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits N_match=975 sigma_overall_arcsec=0.619 sigma_q1_arcsec=0.630 sigma_q2_arcsec=0.593 sigma_q3_arcsec=0.670 sigma_q4_arcsec=0.611 n_q1=330 n_q2=174 n_q3=273 n_q4=198 worst_quadrant_to_overall_ratio=1.082
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-45-43_20.00sec_4.90C_LIGHT_0124.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.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_2026-07-09_CI_Cas-04-Q2b1x1_235431_TTUQ2b1x1_436245_gsq3Oe3q/wcs_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:13:43.57 +53:21:57.3: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:45:04.91 +50:54:58.8: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:22:00.94 +54:12:53.0: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:24:54.44 +53:26:45.2: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:26:37.85 +53:22:52.5: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:15:45.53 +53:37:27.3: 13.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:18.07 +57:21:29.2: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:49.50 +53:38:52.4: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:08:25.45 +52:44:49.8: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:44:27.37 +49:42:04.3: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:13:43.57 +53:21:57.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:22:00.94 +54:12:53.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:45:04.91 +50:54:58.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:37.85 +53:22:52.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:15:45.53 +53:37:27.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:49.50 +53:38:52.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:18.07 +57:21:29.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:08:25.45 +52:44:49.8: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:44:27.37 +49:42:04.3: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:24:54.44 +53:26:45.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:11.15 +56:36:29.2: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:11.15 +56:36:29.2: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:49:13.51 +52:28:15.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:49:13.51 +52:28:15.9: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:13.46 +50:19:54.5: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:11:44.31 +50:55:16.2: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:54:13.46 +50:19:54.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:11:44.31 +50:55:16.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:52:02.79 +55:16:14.3: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:52:02.79 +55:16:14.3: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:38.32 +57:55:03.6: 11.06 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:49:37.84 +56:53:54.7: 11.69 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:38.32 +57:55:03.6: 10.77 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.02
Forced photometry filter REJECTED candidate at 00:30:38.32 +57:55:03.6: ref_mag=10.91 +/- 0.02 new_mean_mag=11.5109 delta=-0.60 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:05.56 +53:23:17.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:48.98 +56:19:34.1: 11.48 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:49:37.84 +56:53:54.7: 11.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.04
Forced photometry filter REJECTED candidate at 23:49:37.84 +56:53:54.7: ref_mag=11.58 +/- 0.04 new_mean_mag=11.3777 delta=0.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:05.56 +53:23:17.9: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:48.98 +56:19:34.1: 11.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.03
Forced photometry filter REJECTED candidate at 23:51:48.98 +56:19:34.1: ref_mag=11.34 +/- 0.03 new_mean_mag=11.2809 delta=0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:10.98 +56:03:03.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:30.11 +52:29:45.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:59.34 +52:05:26.3: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:10.98 +56:03:03.6: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:36.37 +50:36:42.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:30.11 +52:29:45.6: 99.00 +/- 99.00 bad_region
Forced photometry filter REJECTED candidate at 00:29:30.11 +52:29:45.6: the position falls in a bad CCD region (bad_region.lst) on all measured reference images -- cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:59.34 +52:05:26.3: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:40:34.07 +56:55:03.6: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:36.37 +50:36:42.6: 99.00 +/- 99.00 bad_region
Forced photometry filter REJECTED candidate at 00:28:36.37 +50:36:42.6: the position falls in a bad CCD region (bad_region.lst) on all measured reference images -- cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:40:34.07 +56:55:03.6: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:48:06.79 +50:03:10.1: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:36:06.87 +52:01:25.7: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:48:06.79 +50:03:10.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:36:06.87 +52:01:25.7: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:28.49 +55:55:50.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:28.49 +55:55:50.2: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:23:06.53 +53:52:58.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:06.53 +53:52:58.8: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:24.25 +51:41:40.7: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:24.25 +51:41:40.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:58.16 +50:29:55.1: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:54:58.16 +50:29:55.1: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:23.79 +55:49:09.7: 13.45 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:23.79 +55:49:09.7: 13.45 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.45 +/- 0.28
Forced photometry filter KEPT candidate at 00:30:23.79 +55:49:09.7: ref_mag=13.45 +/- 0.28 new_mean_mag=10.9621 delta=2.49 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:53:38.29 +51:20:56.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:53:38.29 +51:20:56.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:03:55.02 +55:04:36.7: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:47.80 +56:39:17.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:03:55.02 +55:04:36.7: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:47.80 +56:39:17.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:01:22.29 +51:04:01.3: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:01:22.29 +51:04:01.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:04.49 +50:59:57.2: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:11.84 +50:30:00.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:04.49 +50:59:57.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:11.84 +50:30:00.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:19:23.42 +54:59:23.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:20:19.19 +56:57:19.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:19:23.42 +54:59:23.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:20:19.19 +56:57:19.9: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:46:36.49 +51:42:15.2: 13.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:36.49 +51:42:15.2: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:03.26 +55:22:32.7: 13.14 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:03.26 +55:22:32.7: 12.66 +/- 0.18 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.14
Forced photometry filter KEPT candidate at 00:29:03.26 +55:22:32.7: ref_mag=12.85 +/- 0.14 new_mean_mag=10.7892 delta=2.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:46.33 +54:50:14.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:46.33 +54:50:14.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:53:14.17 +50:38:36.7: 13.29 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:09.56 +50:24:07.3: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:53:14.17 +50:38:36.7: 12.71 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.13
Forced photometry filter KEPT candidate at 23:53:14.17 +50:38:36.7: ref_mag=12.92 +/- 0.13 new_mean_mag=10.3716 delta=2.55 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:09.56 +50:24:07.3: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:10.83 +56:29:43.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:10.83 +56:29:43.0: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:15:03.76 +51:59:23.5: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:15:03.76 +51:59:23.5: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:14:07.39 +51:33:28.3: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:14:07.39 +51:33:28.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:42.04 +57:00:50.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:42.04 +57:00:50.5: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:23.89 +55:26:50.9: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:23.89 +55:26:50.9: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:32.87 +57:40:50.6: 13.53 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:32.87 +57:40:50.6: 13.31 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.53 +/- 0.33
Forced photometry filter KEPT candidate at 00:19:32.87 +57:40:50.6: ref_mag=13.53 +/- 0.33 new_mean_mag=11.0745 delta=2.46 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:20:17.97 +57:39:09.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:20:17.97 +57:39:09.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:04:13.50 +51:32:55.6: 13.29 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:56.95 +57:43:36.4: 11.07 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:04:13.50 +51:32:55.6: 13.43 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.18
Forced photometry filter KEPT candidate at 00:04:13.50 +51:32:55.6: ref_mag=13.34 +/- 0.18 new_mean_mag=11.1782 delta=2.16 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:56.95 +57:43:36.4: 10.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.86 +/- 0.02
Forced photometry filter REJECTED candidate at 00:31:56.95 +57:43:36.4: ref_mag=10.86 +/- 0.02 new_mean_mag=11.3964 delta=-0.53 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:06:29.46 +50:07:48.1: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:06:29.46 +50:07:48.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:00:49.22 +49:57:54.5: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:00:49.22 +49:57:54.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:21:04.97 +51:45:18.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:21:04.97 +51:45:18.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:00:56.14 +53:53:48.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:00:56.14 +53:53:48.0: 13.46 +/- 99.00 upperlimit
Adding exclusion_list_gaiadr2.txt__out190042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out189886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190493.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 70s
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: 51s
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Considering the candidate 189886_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189886_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189891_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189891_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189894_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189894_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189897_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189897_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189905_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189905_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189913_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189913_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189915_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189915_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189917_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189917_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189923_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189923_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189928_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189928_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
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Considering the candidate 189929_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189929_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:04:21.88 +51:49:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189933_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189933_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:25:16.14 +53:39:16.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189934_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189934_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189936_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189936_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189938_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189938_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:27:56.18 +55:49:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189939_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189939_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189945_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189945_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189947_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189947_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189949_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189949_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189950_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189950_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189951_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189951_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189959_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189959_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189961_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189961_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:01:36.23 +52:04:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189962_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189962_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189973_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189973_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189974_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189974_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189980_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189980_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189981_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189981_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189987_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 189987_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:31:43.18 +56:11:38.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189991_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189991_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189992_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189992_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189993_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189993_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189995_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189995_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189999_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 189999_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190005_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190005_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190006_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190006_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190007_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190007_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:10:30.96 +53:33:33.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190008_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190008_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190011_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190011_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190012_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190012_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190014_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190014_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:57:47.43 +52:08:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190016_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190016_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190017_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190017_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:58:45.13 +54:04:21.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190018_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190018_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190021_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190021_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190024_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190024_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190025_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190025_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190026_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190026_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190027_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190027_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190028_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190028_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:16:11.50 +55:57:19.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190031_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190031_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190035_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190035_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:31:09.93 +55:39:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190042_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190042_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:53:14.17 +50:38:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.40, MAG_FAINT_SEARCH_LIMIT=11.38)GAIADR2_OUTPUT=# 2.568 1944012497231348736 358.30837657107 +50.64410303622 11.1977 10.0555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190043_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190043_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190044_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190044_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190045_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190045_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:14:48.97 +51:48:52.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190046_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190046_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190047_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190047_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:00:53.08 +49:57:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190049_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190049_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:20:50.40 +54:00:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190117_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190117_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:18:59.63 +53:18:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190123_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190123_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:48:52.87 +53:36:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190155_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190155_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190163_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190163_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:10:46.91 +49:57:45.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190166_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190166_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190194_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190194_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:59:23.81 +50:31:41.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190213_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190213_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190278_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190278_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190285_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190285_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:10:01.43 +50:48:48.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190292_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190292_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:57:59.47 +50:26:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190296_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190296_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:26:20.84 +56:46:46.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190303_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190303_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190305_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190305_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:21:25.97 +52:06:38.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190314_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190314_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:09:02.66 +53:08:29.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190317_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190317_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:59:07.26 +53:34:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190321_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190321_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:22:51.11 +52:21:56.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190327_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190327_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:00:20.14 +50:37:34.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190342_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190342_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:43:15.09 +51:56:34.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190348_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190348_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:22:43.28 +52:38:07.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190351_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190351_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190352_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190352_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190355_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190355_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:20:56.54 +56:24:03.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190356_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190356_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:02:36.46 +55:35:41.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190357_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190357_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:10:29.01 +49:51:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190360_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190360_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:05:04.17 +56:02:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190374_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190374_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:13:37.62 +56:24:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190376_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190376_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190387_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190387_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:08:02.12 +53:40:10.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190409_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190409_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:29:00.80 +51:39:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190413_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190413_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190417_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190417_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190442_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190442_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:06:02.09 +51:21:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190468_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190468_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:09:10.31 +53:31:15.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190476_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 190476_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:08:36.87 +55:38:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190493_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
Preparing report for the candidate 190493_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140320_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 140320_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 23:44:31.99 +56:34:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35911_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 35911_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:09:36.52 +51:34:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105722_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125
The candidate 105722_fd_Cas-04-Q2b1x1_2026-07-09_23-47-01_20.00sec_5.00C_LIGHT_0125 did not pass the final checks
**** FOUND 00:04:40.65 +55:32:14.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 127s
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 ####
00:08:25.45 +52:44:49.8
00:17:49.50 +53:38:52.4
00:13:43.57 +53:21:57.3
23:44:27.37 +49:42:04.3
00:15:45.53 +53:37:27.3
00:22:00.94 +54:12:53.0
00:26:37.85 +53:22:52.5
23:45:04.91 +50:54:58.8
00:24:54.44 +53:26:45.2
00:07:18.07 +57:21:29.2
00:31:11.15 +56:36:29.2
23:49:13.51 +52:28:15.9
23:54:13.46 +50:19:54.5
00:11:44.31 +50:55:16.2
23:52:02.79 +55:16:14.3
00:27:05.56 +53:23:17.9
00:29:10.98 +56:03:03.6
00:25:59.34 +52:05:26.3
23:40:34.07 +56:55:03.6
23:48:06.79 +50:03:10.1
23:36:06.87 +52:01:25.7
23:59:28.49 +55:55:50.2
00:23:06.53 +53:52:58.8
23:57:24.25 +51:41:40.7
23:54:58.16 +50:29:55.1
00:30:23.79 +55:49:09.7
23:53:38.29 +51:20:56.6
00:03:55.02 +55:04:36.7
00:28:47.80 +56:39:17.4
00:01:22.29 +51:04:01.3
23:29:04.49 +50:59:57.2
23:58:11.84 +50:30:00.0
23:19:23.42 +54:59:23.2
23:20:19.19 +56:57:19.9
23:46:36.49 +51:42:15.2
00:29:03.26 +55:22:32.7
00:28:46.33 +54:50:14.8
23:57:09.56 +50:24:07.3
00:28:10.83 +56:29:43.0
00:15:03.76 +51:59:23.5
00:14:07.39 +51:33:28.3
00:28:42.04 +57:00:50.5
00:25:23.89 +55:26:50.9
00:19:32.87 +57:40:50.6
00:20:17.97 +57:39:09.9
00:04:13.50 +51:32:55.6
00:06:29.46 +50:07:48.1
00:00:49.22 +49:57:54.5
00:21:04.97 +51:45:18.7
00:00:56.14 +53:53:48.0
########### 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 ####
00:08:25.45 +52:44:49.8
00:17:49.50 +53:38:52.4
00:13:43.57 +53:21:57.3
23:44:27.37 +49:42:04.3
00:15:45.53 +53:37:27.3
00:22:00.94 +54:12:53.0
00:26:37.85 +53:22:52.5
23:45:04.91 +50:54:58.8
00:24:54.44 +53:26:45.2
00:07:18.07 +57:21:29.2
00:31:11.15 +56:36:29.2
23:49:13.51 +52:28:15.9
23:54:13.46 +50:19:54.5
00:11:44.31 +50:55:16.2
23:52:02.79 +55:16:14.3
00:27:05.56 +53:23:17.9
00:29:10.98 +56:03:03.6
00:25:59.34 +52:05:26.3
23:40:34.07 +56:55:03.6
23:48:06.79 +50:03:10.1
23:36:06.87 +52:01:25.7
23:59:28.49 +55:55:50.2
00:23:06.53 +53:52:58.8
23:57:24.25 +51:41:40.7
23:54:58.16 +50:29:55.1
00:30:23.79 +55:49:09.7
23:53:38.29 +51:20:56.6
00:03:55.02 +55:04:36.7
00:28:47.80 +56:39:17.4
00:01:22.29 +51:04:01.3
23:29:04.49 +50:59:57.2
23:58:11.84 +50:30:00.0
23:19:23.42 +54:59:23.2
23:20:19.19 +56:57:19.9
23:46:36.49 +51:42:15.2
00:29:03.26 +55:22:32.7
00:28:46.33 +54:50:14.8
23:57:09.56 +50:24:07.3
00:28:10.83 +56:29:43.0
00:15:03.76 +51:59:23.5
00:14:07.39 +51:33:28.3
00:28:42.04 +57:00:50.5
00:25:23.89 +55:26:50.9
00:19:32.87 +57:40:50.6
00:20:17.97 +57:39:09.9
00:04:13.50 +51:32:55.6
00:06:29.46 +50:07:48.1
00:00:49.22 +49:57:54.5
00:21:04.97 +51:45:18.7
00:00:56.14 +53:53:48.0
###################################################################################
00:08:25.45 +52:44:49.8 -- not an asteroid (will add it to exclusion list)
00:17:49.50 +53:38:52.4 -- not an asteroid (will add it to exclusion list)
00:13:43.57 +53:21:57.3 -- not an asteroid (will add it to exclusion list)
23:44:27.37 +49:42:04.3 -- not an asteroid (will add it to exclusion list)
00:15:45.53 +53:37:27.3 -- not an asteroid (will add it to exclusion list)
00:22:00.94 +54:12:53.0 -- not an asteroid (will add it to exclusion list)
00:26:37.85 +53:22:52.5 -- not an asteroid (will add it to exclusion list)
23:45:04.91 +50:54:58.8 -- not an asteroid (will add it to exclusion list)
00:24:54.44 +53:26:45.2 -- not an asteroid (will add it to exclusion list)
00:07:18.07 +57:21:29.2 -- not an asteroid (will add it to exclusion list)
00:31:11.15 +56:36:29.2 -- not an asteroid (will add it to exclusion list)
23:49:13.51 +52:28:15.9 -- not an asteroid (will add it to exclusion list)
23:54:13.46 +50:19:54.5 -- not an asteroid (will add it to exclusion list)
00:11:44.31 +50:55:16.2 -- not an asteroid (will add it to exclusion list)
23:52:02.79 +55:16:14.3 -- not an asteroid (will add it to exclusion list)
00:27:05.56 +53:23:17.9 -- not an asteroid (will add it to exclusion list)
00:29:10.98 +56:03:03.6 -- not an asteroid (will add it to exclusion list)
00:25:59.34 +52:05:26.3 -- not an asteroid (will add it to exclusion list)
23:40:34.07 +56:55:03.6 -- not an asteroid (will add it to exclusion list)
23:48:06.79 +50:03:10.1 -- not an asteroid (will add it to exclusion list)
23:36:06.87 +52:01:25.7 -- not an asteroid (will add it to exclusion list)
23:59:28.49 +55:55:50.2 -- not an asteroid (will add it to exclusion list)
00:23:06.53 +53:52:58.8 -- not an asteroid (will add it to exclusion list)
23:57:24.25 +51:41:40.7 -- not an asteroid (will add it to exclusion list)
23:54:58.16 +50:29:55.1 -- not an asteroid (will add it to exclusion list)
00:30:23.79 +55:49:09.7 -- not an asteroid (will add it to exclusion list)
23:53:38.29 +51:20:56.6 -- not an asteroid (will add it to exclusion list)
00:03:55.02 +55:04:36.7 -- not an asteroid (will add it to exclusion list)
00:28:47.80 +56:39:17.4 -- not an asteroid (will add it to exclusion list)
00:01:22.29 +51:04:01.3 -- not an asteroid (will add it to exclusion list)
23:29:04.49 +50:59:57.2 -- not an asteroid (will add it to exclusion list)
23:58:11.84 +50:30:00.0 -- not an asteroid (will add it to exclusion list)
23:19:23.42 +54:59:23.2 -- not an asteroid (will add it to exclusion list)
23:20:19.19 +56:57:19.9 -- not an asteroid (will add it to exclusion list)
23:46:36.49 +51:42:15.2 -- not an asteroid (will add it to exclusion list)
00:29:03.26 +55:22:32.7 -- not an asteroid (will add it to exclusion list)
00:28:46.33 +54:50:14.8 -- not an asteroid (will add it to exclusion list)
23:57:09.56 +50:24:07.3 -- not an asteroid (will add it to exclusion list)
00:28:10.83 +56:29:43.0 -- not an asteroid (will add it to exclusion list)
00:15:03.76 +51:59:23.5 -- not an asteroid (will add it to exclusion list)
00:14:07.39 +51:33:28.3 -- not an asteroid (will add it to exclusion list)
00:28:42.04 +57:00:50.5 -- not an asteroid (will add it to exclusion list)
00:25:23.89 +55:26:50.9 -- not an asteroid (will add it to exclusion list)
00:19:32.87 +57:40:50.6 -- not an asteroid (will add it to exclusion list)
00:20:17.97 +57:39:09.9 -- not an asteroid (will add it to exclusion list)
00:04:13.50 +51:32:55.6 -- not an asteroid (will add it to exclusion list)
00:06:29.46 +50:07:48.1 -- not an asteroid (will add it to exclusion list)
00:00:49.22 +49:57:54.5 -- not an asteroid (will add it to exclusion list)
00:21:04.97 +51:45:18.7 -- not an asteroid (will add it to exclusion list)
00:00:56.14 +53:53:48.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:49.22 +49:57:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:00:56.14 +53:53:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:22.29 +51:04:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:55.02 +55:04:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:13.50 +51:32:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:29.46 +50:07:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:18.07 +57:21:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:25.45 +52:44:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:44.31 +50:55:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:43.57 +53:21:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:07.39 +51:33:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:03.76 +51:59:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:45.53 +53:37:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:49.50 +53:38:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:32.87 +57:40:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:17.97 +57:39:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:04.97 +51:45:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:00.94 +54:12:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:06.53 +53:52:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:54.44 +53:26:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:23.89 +55:26:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:59.34 +52:05:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:37.85 +53:22:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:05.56 +53:23:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:10.83 +56:29:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:42.04 +57:00:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:46.33 +54:50:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:47.80 +56:39:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:03.26 +55:22:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:10.98 +56:03:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:23.79 +55:49:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:11.15 +56:36:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:23.42 +54:59:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:19.19 +56:57:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:04.49 +50:59:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:06.87 +52:01:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:34.07 +56:55:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:27.37 +49:42:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:04.91 +50:54:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:36.49 +51:42:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:06.79 +50:03:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:13.51 +52:28:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:02.79 +55:16:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:38.29 +51:20:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:13.46 +50:19:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:58.16 +50:29:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:09.56 +50:24:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:24.25 +51:41:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:11.84 +50:30:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:28.49 +55:55:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:00:49.22 +49:57:54.5 -- not a known variable star
00:00:56.14 +53:53:48.0 -- not a known variable star
00:01:22.29 +51:04:01.3 -- not a known variable star
00:03:55.02 +55:04:36.7 -- not a known variable star
00:04:13.50 +51:32:55.6 -- not a known variable star
00:06:29.46 +50:07:48.1 -- not a known variable star
00:07:18.07 +57:21:29.2 -- not a known variable star
00:08:25.45 +52:44:49.8 -- not a known variable star
00:11:44.31 +50:55:16.2 -- a known variable star
00:13:43.57 +53:21:57.3 -- a known variable star
00:14:07.39 +51:33:28.3 -- not a known variable star
00:15:03.76 +51:59:23.5 -- not a known variable star
00:15:45.53 +53:37:27.3 -- not a known variable star
00:17:49.50 +53:38:52.4 -- not a known variable star
00:19:32.87 +57:40:50.6 -- not a known variable star
00:20:17.97 +57:39:09.9 -- a known variable star
00:21:04.97 +51:45:18.7 -- not a known variable star
00:22:00.94 +54:12:53.0 -- not a known variable star
00:23:06.53 +53:52:58.8 -- not a known variable star
00:24:54.44 +53:26:45.2 -- not a known variable star
00:25:23.89 +55:26:50.9 -- not a known variable star
00:25:59.34 +52:05:26.3 -- not a known variable star
00:26:37.85 +53:22:52.5 -- not a known variable star
00:27:05.56 +53:23:17.9 -- not a known variable star
00:28:10.83 +56:29:43.0 -- not a known variable star
00:28:42.04 +57:00:50.5 -- a known variable star
00:28:46.33 +54:50:14.8 -- a known variable star
00:28:47.80 +56:39:17.4 -- not a known variable star
00:29:03.26 +55:22:32.7 -- a known variable star
00:29:10.98 +56:03:03.6 -- a known variable star
00:30:23.79 +55:49:09.7 -- a known variable star
00:31:11.15 +56:36:29.2 -- a known variable star
23:19:23.42 +54:59:23.2 -- not a known variable star
23:20:19.19 +56:57:19.9 -- a known variable star
23:29:04.49 +50:59:57.2 -- not a known variable star
23:36:06.87 +52:01:25.7 -- not a known variable star
23:40:34.07 +56:55:03.6 -- a known variable star
23:44:27.37 +49:42:04.3 -- not a known variable star
23:45:04.91 +50:54:58.8 -- not a known variable star
23:46:36.49 +51:42:15.2 -- not a known variable star
23:48:06.79 +50:03:10.1 -- not a known variable star
23:49:13.51 +52:28:15.9 -- not a known variable star
23:52:02.79 +55:16:14.3 -- not a known variable star
23:53:38.29 +51:20:56.6 -- not a known variable star
23:54:13.46 +50:19:54.5 -- not a known variable star
23:54:58.16 +50:29:55.1 -- a known variable star
23:57:09.56 +50:24:07.3 -- not a known variable star
23:57:24.25 +51:41:40.7 -- not a known variable star
23:58:11.84 +50:30:00.0 -- not a known variable star
23:59:28.49 +55:55:50.2 -- not a known variable star
Found 38 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
50 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 50 (excluding asteroids and hot pixels, 38 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)2461231.69853844 -observatory V36
07:32:40.14 +17:08:25.7 Mercury (5.0mag)
10:11:00.18 +12:45:00.4 Venus (-4.1mag)
04:23:43.08 +21:24:02.8 Mars (1.3mag)
08:16:32.21 +20:11:55.3 Jupiter (-1.8mag)
00:55:49.88 +03:20:25.2 Saturn (0.7mag)
04:07:12.26 +20:44:58.6 Uranus (5.8mag)
00:17:01.52 +00:20:42.0 Neptune (7.8mag)
20:30:55.78 -23:17:56.5 Pluto (14.4mag)
03:00:50.66 +21:28:32.3 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 361 Jul 10 03:53 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461231.69853844:
08:16:36.37 +20:11:41.8 Io (6.1mag)
08:16:32.37 +20:11:56.4 Europa (6.3mag)
08:16:48.63 +20:10:56.5 Ganymede (5.6mag)
08:17:00.75 +20:10:10.1 Callisto (6.8mag)
08:15:04.13 +19:56:01.0 Himalia (15.7mag)
08:16:30.69 +20:12:01.9 Thebe (16.6mag)
08:14:25.50 +20:00:32.7 Elara (17.6mag)
08:20:04.14 +20:06:10.2 Pasiphae (17.8mag)
08:21:30.58 +20:16:58.9 Carme (19.0mag)
00:55:39.40 +03:20:17.8 Titan (8.5mag)
00:55:44.77 +03:20:30.7 Rhea (9.8mag)
00:55:19.39 +03:19:35.9 Iapetus (11.2mag)
00:55:59.67 +03:20:43.1 Hyperion (14.5mag)
00:55:50.83 +03:17:40.3 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 03:53 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.69853844:
17:46:41.21 -33:02:39.2 JWST
15:53:54.89 +52:41:16.6 Chandra
19:43:34.16 +13:07:03.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 03:53 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.69853844 -observatory V36
02:36:02.99 +14:24:35.1 17.9mag P/1996 R2 (Lagerkvist)
18:18:03.70 -34:21:29.6 13.7mag P/2010 H2 (Vales)
06:25:31.19 -68:08:14.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:45.12 +32:26:39.7 17.6mag C/2017 K2 (PANSTARRS)
17:03:09.65 +16:02:57.4 18.0mag C/2021 G2 (ATLAS)
01:46:54.48 +07:54:34.7 15.4mag P/2021 N1 (ZTF)
22:59:37.35 +32:17:07.8 17.3mag C/2022 E2 (ATLAS)
06:12:13.37 +26:55:39.3 16.7mag C/2022 N2 (PANSTARRS)
09:55:22.88 +29:47:16.1 16.8mag C/2022 QE78 (ATLAS)
09:09:38.15 +04:59:46.3 17.8mag C/2022 R6 (PANSTARRS)
18:07:18.78 +21:17:58.4 17.9mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:36.25 -11:23:03.9 17.7mag P/2023 B1 (PANSTARRS)
21:49:25.17 +67:37:18.2 17.8mag C/2023 H5 (Lemmon)
16:31:11.57 -10:03:43.9 13.9mag C/2023 R1 (PANSTARRS)
08:00:22.99 +65:42:01.3 17.9mag C/2024 A1 (ATLAS)
07:32:36.65 +29:59:43.7 14.6mag C/2024 E1 (Wierzchos)
15:16:24.12 +15:19:27.1 17.5mag C/2024 G6 (ATLAS)
19:41:30.35 +39:21:45.1 13.8mag C/2024 J3 (ATLAS)
21:47:44.41 +45:58:47.2 17.8mag C/2024 R4 (PANSTARRS)
04:49:29.57 -13:48:10.7 15.7mag C/2024 T5 (ATLAS)
06:34:26.62 +29:05:43.4 18.0mag C/2025 J1 (Borisov)
07:14:13.64 -12:52:34.8 16.4mag C/2025 R3 (PANSTARRS)
09:55:54.83 +22:26:36.4 17.6mag C/2025 V2 (Rankin)
12:44:34.02 +03:56:39.3 17.1mag C/2025 Y1 (ATLAS)
16:52:24.19 +79:07:01.0 17.4mag C/2026 A2 (Bok)
02:46:06.51 +45:13:57.8 16.7mag C/2026 B2 (Sun-Gao)
11:25:24.83 +04:30:59.2 16.9mag A/2026 E1
21:18:48.41 -15:01:19.4 7.3mag 10P/Tempel
11:13:23.00 -01:52:50.7 16.1mag 29P/Schwassmann-Wachmann
03:59:56.90 +29:32:10.3 17.8mag 47P/Ashbrook-Jackson
10:07:45.20 +14:03:37.5 17.0mag 63P/Wild
00:48:17.63 -05:05:42.3 15.6mag 65P/Gunn
08:26:28.16 +34:13:33.7 17.9mag 76P/West-Kohoutek-Ikemura
04:27:01.41 +20:10:13.3 13.7mag 78P/Gehrels
02:22:04.87 +10:35:16.0 16.2mag 88P/Howell
06:35:04.06 +30:32:36.2 15.7mag 93P/Lovas
04:20:29.90 +31:06:56.8 16.9mag 114P/Wiseman-Skiff
08:08:18.95 +30:43:13.5 15.3mag 123P/West-Hartley
10:47:50.60 +01:14:58.5 16.8mag 124P/Mrkos
04:51:28.72 +20:48:29.9 16.2mag 128P/Shoemaker-Holt
05:35:57.75 +19:42:53.9 17.8mag 131P/Mueller
00:01:30.14 +02:55:44.4 17.9mag 139P/Vaisala-Oterma
07:12:59.14 +17:03:13.2 15.5mag 141P-D/Machholz
03:16:46.80 -21:07:07.5 15.5mag 161P/Hartley-IRAS
05:32:30.37 +33:54:52.5 15.3mag 162P/SidingSpring
19:04:52.17 +14:59:23.5 14.7mag 169P/NEAT
01:40:39.57 +07:34:50.7 17.7mag 220P/McNaught
16:35:59.78 -08:22:46.8 17.0mag 235P/LINEAR
08:44:57.49 +33:18:49.0 17.9mag 240P/NEAT
20:42:14.84 -49:32:07.6 17.8mag 259P/Garradd
01:58:52.49 +12:01:21.0 15.7mag 260P/McNaught
05:36:45.43 +36:49:48.1 17.4mag 295P/LINEAR
15:06:37.43 +06:04:13.7 17.6mag 391P/Kowalski
08:34:27.87 +19:40:58.8 17.9mag 450P/LONEOS
07:51:31.35 +39:13:44.3 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 03:53 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 10 03:53 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
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
-rw-r--r-- 1 apache apache 189K Jul 10 03:53 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:36:21.258 +13:42:31.91 AT 2026sqg 2026-07-06.96 17.376
10:38:47.961 +53:30:34.10 SN 2026sqf 2026-07-08.25 12.9
13:40:20.447 +40:38:15.61 AT 2026sqe 2026-07-03.20 20.3209
20:26:11.475 -21:05:59.62 AT 2026sqd 2026-07-07.33 20.2909
20:38:05.960 -15:39:19.94 AT 2026sqc 2026-07-07.33 22.2834
21:50:20.218 -14:25:11.02 AT 2026sqb 2026-07-07.39 21.5547
20:32:17.644 -16:37:51.49 AT 2026sqa 2026-07-07.33 21.6569
20:38:02.144 -16:39:15.94 AT 2026spz 2026-07-07.33 22.7762
20:36:24.191 -15:13:43.37 AT 2026spy 2026-07-07.33 22.1739
20:41:10.988 -25:49:45.49 AT 2026spx 2026-07-07.33 22.8645
21:17:15.336 -23:31:53.39 AT 2026spw 2026-07-07.32 21.9459
20:27:45.431 -19:59:58.81 AT 2026spv 2026-07-07.33 21.6485
21:55:34.604 -14:11:57.66 AT 2026spu 2026-07-07.39 23.0585
21:10:34.181 -22:59:24.76 AT 2026spt 2026-07-07.32 22.3526
21:05:55.405 -19:04:02.26 AT 2026sps 2026-07-07.32 21.4424
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
20:31:34.503 -19:06:25.71 AT 2026spq 2026-07-07.33 22.7105
20:54:43.024 -26:43:41.99 AT 2026spp 2026-07-07.32 22.8017
21:07:49.748 -22:55:35.56 AT 2026spo 2026-07-07.32 22.494
20:57:55.962 -26:08:04.97 AT 2026spn 2026-07-07.32 22.7486
-rw-r--r-- 1 apache apache 30K Jul 10 03:53 tns_transients_list.txt
