This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi
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 11.1958 2461232.6958 10.15 00:46:45.10 +58:10:06.7
122.31196 -4.69758 galactic Cas Second-epoch detections are separated by 1.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J011.6901+58.1714 | 00:46:44.99 +58:10:06.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.669+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:45.10 +58:10:06.7: 11.90 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:45.10 +58:10:06.7: 11.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 00 46 45.10 +58 10 06.7 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
ATO J011.6901+58.1714,2461232.6958,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J011.6901+58.1714 20260711.1958 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.88 00:53:07.33 +54:59:08.3
123.17582 -7.88531 galactic Cas Second-epoch detections are separated by 1.2" and 3.0 pix
The object was found in VSX 1" TYC 3659-550-1
Type: EW
# Max. Min./Amp. JD0 Period
11.410 V 11.500 V 2458097.98400 0.275862000000 F5
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:53:07.33 +54:59:08.3: 12.52 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:53:07.33 +54:59:08.3: 12.13 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 00 53 07.33 +54 59 08.3 9.9 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
TYC 3659-550-1,2461232.6958,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TYC 3659-550-1 20260711.1958 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.81 23:53:15.27 +50:38:28.6
113.58846 -11.17192 galactic Cas Second-epoch detections are separated by 1.8" and 3.0 pix
The object was found in VSX16" ASASSN-V J235314.01+503838.8
Type: SR
# Max. Min./Amp. JD0 Period
11.790 V 11.900 V 2457177.00000 846.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:53:15.27 +50:38:28.6: 12.70 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:53:15.27 +50:38:28.6: 12.51 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 23 53 15.27 +50 38 28.6 9.8 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
ASASSN-V J235314.01+503838.8,2461232.6958,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J235314.01+503838.8 20260711.1958 9.81CV 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 11.1958 2461232.6958 7.33 00:47:13.23 +50:39:03.9
122.24795 -12.21506 galactic Cas Second-epoch detections are separated by 1.0" and 3.4 pix
The object was found in VSX22" Gaia DR3 415178992264005632
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
8.460 G 8.500 G 1.185000000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:13.23 +50:39:03.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:13.23 +50:39:03.9: 13.12 +/- 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 11.1958* 00 47 13.23 +50 39 03.9 7.3 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 415178992264005632,2461232.6958,7.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 415178992264005632 20260711.1958 7.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 8.36 00:57:24.05 +57:00:14.0
123.74794 -5.85841 galactic Cas Second-epoch detections are separated by 0.4" and 2.8 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 J014.3606+57.0129 | 00:57:24.26 +57:00:15.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.209+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:57:24.05 +57:00:14.0: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:57:24.05 +57:00:14.0: 13.07 +/- 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 11.1958* 00 57 24.05 +57 00 14.0 8.4 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 J014.3606+57.0129,2461232.6958,8.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J014.3606+57.0129 20260711.1958 8.36CV 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 11.1958 2461232.6958 9.57 00:38:23.41 +48:47:52.8
120.71792 -14.01765 galactic Cas Second-epoch detections are separated by 2.6" and 3.3 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 391289735627775744 | 00:38:23.70 +48:47:59.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:23.41 +48:47:52.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:23.41 +48:47:52.8: 13.20 +/- 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 11.1958* 00 38 23.41 +48 47 52.8 9.6 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 391289735627775744,2461232.6958,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 391289735627775744 20260711.1958 9.57CV 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 11.1958 2461232.6958 10.02 00:56:51.93 +57:23:42.4
123.66637 -5.46890 galactic Cas Second-epoch detections are separated by 1.3" and 2.6 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 J014.1842+57.3974 | 00:56:47.94 +57:23:58.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.271+/-0.032 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:56:51.93 +57:23:42.4: 11.62 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:56:51.93 +57:23:42.4: 11.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 00 56 51.93 +57 23 42.4 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 J014.1842+57.3974,2461232.6958,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J014.1842+57.3974 20260711.1958 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.79 00:34:01.07 +48:38:59.6
119.96661 -14.12154 galactic Cas Second-epoch detections are separated by 2.0" and 3.8 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 390962218599996544 | 00:34:01.64 +48:39:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:01.07 +48:38:59.6: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:01.07 +48:38:59.6: 13.21 +/- 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 11.1958* 00 34 01.07 +48 38 59.6 9.8 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 390962218599996544,2461232.6958,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 390962218599996544 20260711.1958 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.07 23:59:23.37 +50:31:39.3
114.53310 -11.49345 galactic Cas Second-epoch detections are separated by 5.6" and 3.7 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 1940961485601981312 | 23:59:23.77 +50:31:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:23.37 +50:31:39.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:23.37 +50:31:39.3: 13.44 +/- 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 11.1958* 23 59 23.37 +50 31 39.3 10.1 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 1940961485601981312,2461232.6958,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940961485601981312 20260711.1958 10.07CV 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 11.1958 2461232.6958 10.21 00:34:32.88 +48:52:56.4
120.07287 -13.89563 galactic Cas Second-epoch detections are separated by 4.1" and 3.8 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 391329038867641600 | 00:34:33.08 +48:52:59.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:32.88 +48:52:56.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:32.88 +48:52:56.4: 13.24 +/- 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 11.1958* 00 34 32.88 +48 52 56.4 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 391329038867641600,2461232.6958,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 391329038867641600 20260711.1958 10.21CV 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 11.1958 2461232.6958 10.59 23:59:25.41 +57:41:21.0
116.00284 -4.48113 galactic Cas Second-epoch detections are separated by 2.5" and 2.5 pix
The object was found in VSX 1" ASASSN-V J235925.48+574122.0
Type: SR
# Max. Min./Amp. JD0 Period
13.320 V 13.410 V 2457603.00000 646.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:25.41 +57:41:21.0: 13.15 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:25.41 +57:41:21.0: 12.77 +/- 0.20 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 11.1958* 23 59 25.41 +57 41 21.0 10.6 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
ASASSN-V J235925.48+574122.0,2461232.6958,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J235925.48+574122.0 20260711.1958 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.55 00:05:07.08 +59:04:42.3
117.00165 -3.25896 galactic Cas Second-epoch detections are separated by 3.1" and 3.2 pix
The object was found in VSX 3" ZTF J000507.41+590443.4
Type: SR
# Max. Min./Amp. JD0 Period
13.710 r Y 0.154 r 2458348.48900 70.101046300000
ATTENTION: measured mag 10.55 is 3.0 mag brighter than the VSX record maximum brightness 13.56 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:05:07.08 +59:04:42.3: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:05:07.08 +59:04:42.3: 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 11.1958* 00 05 07.08 +59 04 42.3 10.6 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
ZTF J000507.41+590443.4,2461232.6958,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J000507.41+590443.4 20260711.1958 10.55CV 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 11.1958 2461232.6958 10.45 00:18:13.02 +51:33:59.2
117.68436 -10.96650 galactic Cas Second-epoch detections are separated by 2.2" and 2.9 pix
The object was found in VSX 1" ASASSN-V J001812.95+513358.7
Type: SR
# Max. Min./Amp. JD0 Period
13.080 V 13.750 V 2458383.22370 56.115624400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:18:13.02 +51:33:59.2: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:18:13.02 +51:33:59.2: 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 11.1958* 00 18 13.02 +51 33 59.2 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 J001812.95+513358.7,2461232.6958,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J001812.95+513358.7 20260711.1958 10.45CV 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 11.1958 2461232.6958 10.69 23:58:33.06 +58:30:07.0
116.05460 -3.66184 galactic Cas Second-epoch detections are separated by 1.0" and 2.9 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 | 23:58:33.06 +58:30:07.0 (user input) | T | P | (position from user input) J-Ks=0.814+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:33.06 +58:30:07.0: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:33.06 +58:30:07.0: 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 11.1958* 23 58 33.06 +58 30 07.0 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
target,2461232.6958,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.69CV 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 11.1958 2461232.6958 10.54 23:29:15.29 +53:00:21.8
110.62203 -7.89020 galactic Cas Second-epoch detections are separated by 3.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:29:15.29 +53:00:21.8 (user input) | T | P | (position from user input) J-Ks=0.659+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:15.29 +53:00:21.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:15.29 +53:00:21.8: 13.46 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 23 29 15.29 +53 00 21.8 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
target,2461232.6958,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.70 23:28:09.90 +52:46:46.7
110.39206 -8.05274 galactic Cas Second-epoch detections are separated by 1.2" and 3.1 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 1992478420027480448 | 23:28:09.84 +52:46:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.163+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:09.90 +52:46:46.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:09.90 +52:46:46.7: 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 11.1958* 23 28 09.90 +52 46 46.7 9.7 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 1992478420027480448,2461232.6958,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992478420027480448 20260711.1958 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.59 23:28:17.33 +52:53:23.5
110.44549 -7.95425 galactic Cas Second-epoch detections are separated by 2.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:17.33 +52:53:23.5 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:17.33 +52:53:23.5: 13.02 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:17.33 +52:53:23.5: 13.17 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 23 28 17.33 +52 53 23.5 10.6 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,2461232.6958,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.39 23:56:50.84 +58:46:38.8
115.89453 -3.34640 galactic Cas Second-epoch detections are separated by 1.3" and 2.5 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 J359.2115+58.7776 | 23:56:50.77 +58:46:39.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.456+/-0.023 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:56:50.84 +58:46:38.8: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:56:50.84 +58:46:38.8: 13.39 +/- 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 11.1958* 23 56 50.84 +58 46 38.8 9.4 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 J359.2115+58.7776,2461232.6958,9.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.2115+58.7776 20260711.1958 9.39CV 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 11.1958 2461232.6958 10.80 23:58:45.64 +58:13:24.7
116.02477 -3.94002 galactic Cas Second-epoch detections are separated by 3.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:45.64 +58:13:24.7 (user input) | T | P | (position from user input) J-Ks=0.837+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:45.64 +58:13:24.7: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:45.64 +58:13:24.7: 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 11.1958* 23 58 45.64 +58 13 24.7 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
target,2461232.6958,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.71 23:58:45.25 +58:31:38.5
116.08581 -3.64236 galactic Cas Second-epoch detections are separated by 2.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:45.25 +58:31:38.5 (user input) | T | P | (position from user input) J-Ks=0.926+/-0.031 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:45.25 +58:31:38.5: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:45.25 +58:31:38.5: 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 11.1958* 23 58 45.25 +58 31 38.5 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
target,2461232.6958,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.44 23:57:56.96 +58:50:00.9
116.04604 -3.32121 galactic Cas Second-epoch detections are separated by 1.1" and 2.9 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 | 23:57:56.96 +58:50:00.9 (user input) | T | P | (position from user input) J-Ks=0.655+/-0.034 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:56.96 +58:50:00.9: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:56.96 +58:50:00.9: 13.51 +/- 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 11.1958* 23 57 56.96 +58 50 00.9 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
target,2461232.6958,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.12 23:57:59.33 +58:54:44.1
116.06729 -3.24528 galactic Cas Second-epoch detections are separated by 1.5" and 2.6 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 J359.5084+58.9148 | 23:57:59.32 +58:54:44.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.687+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:59.33 +58:54:44.1: 13.11 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:59.33 +58:54:44.1: 13.41 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.11 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 11.1958* 23 57 59.33 +58 54 44.1 9.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.5084+58.9148,2461232.6958,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.5084+58.9148 20260711.1958 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.35 23:58:40.44 +58:21:10.3
116.03996 -3.81108 galactic Cas Second-epoch detections are separated by 1.1" and 2.9 pix
The object was found in VSX 1" V0543 Cas
Type: LB:
# Max. Min./Amp. JD0 Period
16.600 B 17.100 B 274.000000000000 C
ATTENTION: measured mag 9.35 is 7.3 mag brighter than the VSX record maximum brightness 16.60 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:40.44 +58:21:10.3: 12.82 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:40.44 +58:21:10.3: 12.40 +/- 0.15 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 23 58 40.44 +58 21 10.3 9.3 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
V0543 Cas,2461232.6958,9.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0543 Cas 20260711.1958 9.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.73 23:58:03.21 +58:55:46.3
116.07903 -3.23009 galactic Cas Second-epoch detections are separated by 2.3" and 2.4 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 J359.5246+58.9194 | 23:58:03.21 +58:55:46.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.290+/-0.036 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:03.21 +58:55:46.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:03.21 +58:55:46.3: 13.36 +/- 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 11.1958* 23 58 03.21 +58 55 46.3 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
ATO J359.5246+58.9194,2461232.6958,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.5246+58.9194 20260711.1958 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 11.1958 2461232.6958 10.28 23:29:10.70 +53:03:34.8
110.62808 -7.83570 galactic Cas Second-epoch detections are separated by 1.0" and 3.2 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 | 23:29:10.70 +53:03:34.8 (user input) | T | P | (position from user input) J-Ks=0.764+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:10.70 +53:03:34.8: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:10.70 +53:03:34.8: 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 11.1958* 23 29 10.70 +53 03 34.8 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461232.6958,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 8.85 23:56:44.76 +58:48:59.3
115.88991 -3.30548 galactic Cas Second-epoch detections are separated by 1.6" and 2.6 pix
The object was found in VSX 4" IRAS 23542+5832
Type: SRB
# Max. Min./Amp. JD0 Period
12.900 V 13.700 V 2457666.00000 58.800000000000 M5e
ATTENTION: measured mag 8.85 is 4.1 mag brighter than the VSX record maximum brightness 12.90 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:56:44.76 +58:48:59.3: 12.19 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:56:44.76 +58:48:59.3: 11.84 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 23 56 44.76 +58 48 59.3 8.8 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
IRAS 23542+5832,2461232.6958,8.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IRAS 23542+5832 20260711.1958 8.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.30 23:28:48.93 +53:06:42.1
110.59252 -7.76911 galactic Cas Second-epoch detections are separated by 0.9" and 3.0 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 1992534456462955392 | 23:28:48.89 +53:06:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.048+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:48.93 +53:06:42.1: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:48.93 +53:06:42.1: 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 11.1958* 23 28 48.93 +53 06 42.1 10.3 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 1992534456462955392,2461232.6958,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992534456462955392 20260711.1958 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.57 23:58:11.05 +58:57:41.5
116.10213 -3.20224 galactic Cas Second-epoch detections are separated by 0.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:11.05 +58:57:41.5 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.374+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:11.05 +58:57:41.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:11.05 +58:57:41.5: 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 11.1958* 23 58 11.05 +58 57 41.5 10.6 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,2461232.6958,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.57CV 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 11.1958 2461232.6958 9.69 23:07:35.41 +54:21:27.8
108.08262 -5.49250 galactic Cas Second-epoch detections are separated by 1.4" and 3.4 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 J346.8970+54.3577 | 23:07:35.28 +54:21:27.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.217+/-0.041 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:07:35.41 +54:21:27.8: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:07:35.41 +54:21:27.8: 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 11.1958* 23 07 35.41 +54 21 27.8 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J346.8970+54.3577,2461232.6958,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J346.8970+54.3577 20260711.1958 9.69CV 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 11.1958 2461232.6958 9.39 23:58:31.98 +59:00:19.1
116.15516 -3.16858 galactic Cas Second-epoch detections are separated by 0.5" and 2.6 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 1999238458034809344 | 23:58:31.79 +59:00:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.053+/-0.034 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:31.98 +59:00:19.1: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:31.98 +59:00:19.1: 13.40 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 11.1958* 23 58 31.98 +59 00 19.1 9.4 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 1999238458034809344,2461232.6958,9.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999238458034809344 20260711.1958 9.39CV 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 11.1958 2461232.6958 10.50 23:28:57.10 +53:04:00.0
110.59770 -7.81829 galactic Cas Second-epoch detections are separated by 3.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:57.10 +53:04:00.0 (user input) | T | P | (position from user input) J-Ks=0.886+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:57.10 +53:04:00.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:57.10 +53:04:00.0: 13.40 +/- 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 11.1958* 23 28 57.10 +53 04 00.0 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
target,2461232.6958,10.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.76 23:58:06.83 +58:53:50.9
116.08006 -3.26307 galactic Cas Second-epoch detections are separated by 1.4" and 2.6 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 1999225534470428544 | 23:58:06.81 +58:53:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.425+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:06.83 +58:53:50.9: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:06.83 +58:53:50.9: 13.40 +/- 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 11.1958* 23 58 06.83 +58 53 50.9 9.8 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 1999225534470428544,2461232.6958,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999225534470428544 20260711.1958 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.81 23:58:23.43 +58:53:22.8
116.11349 -3.27803 galactic Cas Second-epoch detections are separated by 0.5" and 2.8 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 1999224641117231360 | 23:58:23.30 +58:53:23.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:23.43 +58:53:22.8: 13.52 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:23.43 +58:53:22.8: 13.49 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.52 +/- 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 11.1958* 23 58 23.43 +58 53 22.8 9.8 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 1999224641117231360,2461232.6958,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999224641117231360 20260711.1958 9.81CV 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 11.1958 2461232.6958 10.89 23:59:18.28 +59:01:10.2
116.25545 -3.17479 galactic Cas Second-epoch detections are separated by 1.4" and 2.6 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 J359.8153+59.0147 | 23:59:18.28 +59:01:10.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.899+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:18.28 +59:01:10.2: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:18.28 +59:01:10.2: 13.44 +/- 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 11.1958* 23 59 18.28 +59 01 10.2 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
ATO J359.8153+59.0147,2461232.6958,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.8153+59.0147 20260711.1958 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.27 23:59:19.21 +58:18:04.8
116.11276 -3.87870 galactic Cas Second-epoch detections are separated by 0.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:59:19.21 +58:18:04.8 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:19.21 +58:18:04.8: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:19.21 +58:18:04.8: 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 11.1958* 23 59 19.21 +58 18 04.8 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461232.6958,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.27CV 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 11.1958 2461232.6958 10.47 23:57:56.61 +58:49:24.5
116.04322 -3.33095 galactic Cas Second-epoch detections are separated by 1.5" and 2.9 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 | 23:57:56.61 +58:49:24.5 (user input) | T | P | (position from user input) J-Ks=0.242+/-0.037 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:56.61 +58:49:24.5: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:56.61 +58:49:24.5: 13.51 +/- 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 11.1958* 23 57 56.61 +58 49 24.5 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
target,2461232.6958,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.73 23:57:57.33 +58:59:11.1
116.07838 -3.17182 galactic Cas Second-epoch detections are separated by 1.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:57:57.33 +58:59:11.1 (user input) | T | P | (position from user input) J-Ks=0.826+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:57.33 +58:59:11.1: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:57.33 +58:59:11.1: 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 11.1958* 23 57 57.33 +58 59 11.1 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
target,2461232.6958,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 11.1958 2461232.6958 9.45 23:57:44.20 +58:54:10.6
116.03346 -3.24767 galactic Cas Second-epoch detections are separated by 1.0" and 2.6 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 1999219968192812800 | 23:57:44.13 +58:54:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.471+/-0.034 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:44.20 +58:54:10.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:44.20 +58:54:10.6: 13.32 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 23 57 44.20 +58 54 10.6 9.4 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 1999219968192812800,2461232.6958,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999219968192812800 20260711.1958 9.45CV 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 11.1958 2461232.6958 10.05 23:58:04.28 +59:00:23.5
116.09715 -3.15521 galactic Cas Second-epoch detections are separated by 2.0" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:04.28 +59:00:23.5 (user input) | T | P | (position from user input) J-Ks=0.464+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:04.28 +59:00:23.5: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:04.28 +59:00:23.5: 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 11.1958* 23 58 04.28 +59 00 23.5 10.1 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,2461232.6958,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.28 23:58:38.70 +58:17:04.5
116.02229 -3.87715 galactic Cas Second-epoch detections are separated by 1.2" and 2.5 pix
The object was found in VSX 1" Gaia DR3 1998394857738847616
Type: ROT
# Max. Min./Amp. JD0 Period
12.680 G 12.710 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:38.70 +58:17:04.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:38.70 +58:17:04.5: 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 11.1958* 23 58 38.70 +58 17 04.5 10.3 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 1998394857738847616,2461232.6958,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998394857738847616 20260711.1958 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.57 23:58:14.26 +58:40:19.1
116.04941 -3.48706 galactic Cas Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:14.26 +58:40:19.1 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:14.26 +58:40:19.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:14.26 +58:40:19.1: 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 11.1958* 23 58 14.26 +58 40 19.1 10.6 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,2461232.6958,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.57CV 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 11.1958 2461232.6958 10.55 23:28:56.07 +52:50:39.8
110.52420 -8.02833 galactic Cas Second-epoch detections are separated by 2.3" and 3.4 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 J352.2262+52.8523 | 23:28:56.07 +52:50:39.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.354+/-0.031 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:56.07 +52:50:39.8: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:56.07 +52:50:39.8: 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 11.1958* 23 28 56.07 +52 50 39.8 10.6 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
ATO J352.2262+52.8523,2461232.6958,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.2262+52.8523 20260711.1958 10.55CV 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 11.1958 2461232.6958 10.51 23:59:09.54 +58:55:51.4
116.21918 -3.25776 galactic Cas Second-epoch detections are separated by 2.2" and 2.4 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 1999223683347363584 | 23:59:09.54 +58:55:52.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.317+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:09.54 +58:55:51.4: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:09.54 +58:55:51.4: 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 11.1958* 23 59 09.54 +58 55 51.4 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 1999223683347363584,2461232.6958,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999223683347363584 20260711.1958 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.45 23:59:11.84 +58:16:00.5
116.08994 -3.90927 galactic Cas Second-epoch detections are separated by 1.0" and 2.9 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 | 23:59:11.84 +58:16:00.5 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:11.84 +58:16:00.5: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:11.84 +58:16:00.5: 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 11.1958* 23 59 11.84 +58 16 00.5 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
target,2461232.6958,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.45CV 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 11.1958 2461232.6958 10.56 23:58:33.79 +58:57:20.5
116.14884 -3.21794 galactic Cas Second-epoch detections are separated by 1.8" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:33.79 +58:57:20.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:33.79 +58:57:20.5: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:33.79 +58:57:20.5: 13.47 +/- 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 11.1958* 23 58 33.79 +58 57 20.5 10.6 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,2461232.6958,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.35 23:28:07.43 +52:44:24.5
110.37336 -8.08817 galactic Cas Second-epoch detections are separated by 2.6" and 3.3 pix
The object was found in VSX 6" Gaia DR3 1992475327651032832
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.760 G G
ATTENTION: measured mag 10.35 is 3.4 mag brighter than the VSX record maximum brightness 13.74 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:07.43 +52:44:24.5: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:07.43 +52:44:24.5: 13.47 +/- 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 11.1958* 23 28 07.43 +52 44 24.5 10.3 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 1992475327651032832,2461232.6958,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992475327651032832 20260711.1958 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.72 00:00:13.60 +59:04:12.5
116.38192 -3.14880 galactic Cas Second-epoch detections are separated by 0.6" and 2.8 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 423153513884641664 | 00:00:13.61 +59:04:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.841+/-0.032 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:00:13.60 +59:04:12.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:00:13.60 +59:04:12.5: 13.30 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 11.1958* 00 00 13.60 +59 04 12.5 9.7 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 423153513884641664,2461232.6958,9.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 423153513884641664 20260711.1958 9.72CV 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 11.1958 2461232.6958 10.20 23:59:06.93 +58:59:45.4
116.22681 -3.19296 galactic Cas Second-epoch detections are separated by 2.0" and 2.8 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 J359.7788+58.9965 | 23:59:06.93 +58:59:45.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.310+/-0.035 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:06.93 +58:59:45.4: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:06.93 +58:59:45.4: 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 11.1958* 23 59 06.93 +58 59 45.4 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
ATO J359.7788+58.9965,2461232.6958,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.7788+58.9965 20260711.1958 10.20CV 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 11.1958 2461232.6958 10.74 23:28:03.34 +52:46:31.9
110.37491 -8.05135 galactic Cas Second-epoch detections are separated by 4.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:03.34 +52:46:31.9 (user input) | T | P | (position from user input) J-Ks=0.760+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:03.34 +52:46:31.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:03.34 +52:46:31.9: 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 11.1958* 23 28 03.34 +52 46 31.9 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
target,2461232.6958,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.69 23:58:04.26 +59:01:35.4
116.10122 -3.13566 galactic Cas Second-epoch detections are separated by 1.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:04.26 +59:01:35.4 (user input) | T | P | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.197+/-0.035 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:04.26 +59:01:35.4: 13.16 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:04.26 +59:01:35.4: 12.64 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 23 58 04.26 +59 01 35.4 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
target,2461232.6958,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.69CV 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 11.1958 2461232.6958 10.44 23:58:30.65 +59:01:43.7
116.15716 -3.14500 galactic Cas Second-epoch detections are separated by 2.2" and 2.4 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 | Large-amplitude variable Gaia DR2 1999239248308913664 | 23:58:30.65 +59:01:43.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F0 (LAMOST DR5) J-Ks=0.319+/-0.031 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:30.65 +59:01:43.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:30.65 +59:01:43.7: 13.47 +/- 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 11.1958* 23 58 30.65 +59 01 43.7 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
Large-amplitude variable Gaia DR2 1999239248308913664,2461232.6958,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1999239248308913664 20260711.1958 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.38 23:28:38.04 +52:52:58.2
110.49307 -7.97748 galactic Cas Second-epoch detections are separated by 1.1" and 3.1 pix
The object was found in VSX24" Gaia DR3 1992481237526165888
Type: ROT
# Max. Min./Amp. JD0 Period
15.730 G 15.760 G G
ATTENTION: measured mag 10.38 is 5.3 mag brighter than the VSX record maximum brightness 15.73 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:38.04 +52:52:58.2: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:38.04 +52:52:58.2: 13.32 +/- 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 11.1958* 23 28 38.04 +52 52 58.2 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 1992481237526165888,2461232.6958,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992481237526165888 20260711.1958 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.70 23:29:02.71 +52:51:28.6
110.54453 -8.02075 galactic Cas Second-epoch detections are separated by 1.1" and 3.3 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 | Large-amplitude variable Gaia DR2 1992477629750126848 | 23:29:02.77 +52:51:28.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.713+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:02.71 +52:51:28.6: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:02.71 +52:51:28.6: 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 11.1958* 23 29 02.71 +52 51 28.6 9.7 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
Large-amplitude variable Gaia DR2 1992477629750126848,2461232.6958,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1992477629750126848 20260711.1958 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.64 23:57:18.68 +58:30:47.8
115.89821 -3.61735 galactic Cas Second-epoch detections are separated by 0.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:57:18.68 +58:30:47.8 (user input) | T | P | (position from user input) J-Ks=1.219+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:18.68 +58:30:47.8: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:18.68 +58:30:47.8: 13.51 +/- 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 11.1958* 23 57 18.68 +58 30 47.8 10.6 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,2461232.6958,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.64CV 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 11.1958 2461232.6958 10.66 00:07:31.32 +58:56:22.5
117.28264 -3.44963 galactic Cas Second-epoch detections are separated by 2.3" and 3.0 pix
The object was found in VSX 2" ZTF J000731.52+585624.1
Type: SR
# Max. Min./Amp. JD0 Period
14.575 g Y 0.104 g 2458408.26150 289.436197200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:31.32 +58:56:22.5: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:31.32 +58:56:22.5: 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 11.1958* 00 07 31.32 +58 56 22.5 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
ZTF J000731.52+585624.1,2461232.6958,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J000731.52+585624.1 20260711.1958 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 11.1958 2461232.6958 9.94 23:58:45.77 +58:45:41.4
116.13458 -3.41333 galactic Cas Second-epoch detections are separated by 0.4" and 2.7 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 1998468967391319936 | 23:58:45.82 +58:45:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.986+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:45.77 +58:45:41.4: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:45.77 +58:45:41.4: 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 11.1958* 23 58 45.77 +58 45 41.4 9.9 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 1998468967391319936,2461232.6958,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998468967391319936 20260711.1958 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.17 23:59:26.31 +58:59:27.8
116.26664 -3.20612 galactic Cas Second-epoch detections are separated by 0.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J359.8566+58.9941 | 23:59:26.31 +58:59:27.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:26.31 +58:59:27.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:26.31 +58:59:27.8: 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 11.1958* 23 59 26.31 +58 59 27.8 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
ATO J359.8566+58.9941,2461232.6958,10.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.8566+58.9941 20260711.1958 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.60 23:59:19.41 +58:22:25.9
116.12781 -3.80774 galactic Cas Second-epoch detections are separated by 1.4" and 2.5 pix
The object was found in VSX 8" Gaia DR3 1998396880662318464
Type: E
# Max. Min./Amp. JD0 Period
18.620 G 18.780 G 0.468501000000
ATTENTION: measured mag 10.60 is 8.0 mag brighter than the VSX record maximum brightness 18.62 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:19.41 +58:22:25.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:19.41 +58:22:25.9: 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 11.1958* 23 59 19.41 +58 22 25.9 10.6 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 1998396880662318464,2461232.6958,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998396880662318464 20260711.1958 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.49 23:28:35.58 +53:06:43.8
110.56071 -7.75807 galactic Cas Second-epoch detections are separated by 0.8" and 3.0 pix
The object was found in VSX24" Gaia DR3 1992534323323297792
Type: ROT
# Max. Min./Amp. JD0 Period
15.740 G 15.780 G G
ATTENTION: measured mag 10.49 is 5.2 mag brighter than the VSX record maximum brightness 15.74 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:35.58 +53:06:43.8: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:35.58 +53:06:43.8: 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 11.1958* 23 28 35.58 +53 06 43.8 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 1992534323323297792,2461232.6958,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992534323323297792 20260711.1958 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.67 23:29:14.41 +52:57:59.6
110.60733 -7.92699 galactic Cas Second-epoch detections are separated by 4.3" and 3.7 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 J352.3091+52.9666 | 23:29:14.41 +52:57:59.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.057 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:14.41 +52:57:59.6: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:14.41 +52:57:59.6: 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 11.1958* 23 29 14.41 +52 57 59.6 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
ATO J352.3091+52.9666,2461232.6958,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.3091+52.9666 20260711.1958 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 11.1958 2461232.6958 10.14 23:58:31.80 +58:55:54.6
116.13977 -3.24043 galactic Cas Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:31.80 +58:55:54.6 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:31.80 +58:55:54.6: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:31.80 +58:55:54.6: 13.22 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 11.1958* 23 58 31.80 +58 55 54.6 10.1 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,2461232.6958,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.14CV 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 11.1958 2461232.6958 10.16 23:28:54.38 +52:54:18.8
110.53958 -7.96928 galactic Cas Second-epoch detections are separated by 0.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.2298+52.9081 | 23:28:54.38 +52:54:18.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:54.38 +52:54:18.8: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:54.38 +52:54:18.8: 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 11.1958* 23 28 54.38 +52 54 18.8 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
ATO J352.2298+52.9081,2461232.6958,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.2298+52.9081 20260711.1958 10.16CV 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 11.1958 2461232.6958 10.34 23:58:37.32 +59:04:45.3
116.18147 -3.09852 galactic Cas Second-epoch detections are separated by 1.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:37.32 +59:04:45.3 (user input) | T | P | (position from user input) J-Ks=0.262+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:37.32 +59:04:45.3: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:37.32 +59:04:45.3: 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 11.1958* 23 58 37.32 +59 04 45.3 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461232.6958,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.22 23:58:20.45 +59:00:01.9
116.12993 -3.16821 galactic Cas Second-epoch detections are separated by 0.5" and 2.7 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 1999238114437423744 | 23:58:20.47 +59:00:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1955IzKry..14....3B [B55b] 5342 J-Ks=0.218+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:20.45 +59:00:01.9: 13.49 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:20.45 +59:00:01.9: 13.39 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 11.1958* 23 58 20.45 +59 00 01.9 9.2 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 1999238114437423744,2461232.6958,9.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999238114437423744 20260711.1958 9.22CV 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 11.1958 2461232.6958 10.11 00:49:29.57 +52:12:07.4
122.62865 -10.66855 galactic Cas Second-epoch detections are separated by 2.1" and 3.3 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 J012.3801+52.1993 | 00:49:29.62 +52:12:07.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.582+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:49:29.57 +52:12:07.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:49:29.57 +52:12:07.4: 13.24 +/- 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 11.1958* 00 49 29.57 +52 12 07.4 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J012.3801+52.1993,2461232.6958,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J012.3801+52.1993 20260711.1958 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.76 23:58:12.86 +58:41:57.9
116.05207 -3.45957 galactic Cas Second-epoch detections are separated by 2.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:12.86 +58:41:57.9 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:12.86 +58:41:57.9: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:12.86 +58:41:57.9: 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 11.1958* 23 58 12.86 +58 41 57.9 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
target,2461232.6958,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.76CV 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 11.1958 2461232.6958 9.74 23:28:56.63 +52:49:22.8
110.51871 -8.04906 galactic Cas Second-epoch detections are separated by 1.3" and 3.4 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 J352.2393+52.8250 | 23:28:56.63 +52:49:22.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:56.63 +52:49:22.8: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:56.63 +52:49:22.8: 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 11.1958* 23 28 56.63 +52 49 22.8 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.2393+52.8250,2461232.6958,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.2393+52.8250 20260711.1958 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.24 00:00:22.12 +59:04:43.1
116.40151 -3.14406 galactic Cas Second-epoch detections are separated by 0.8" and 2.8 pix
The object was found in VSX 1" ZTF J000022.06+590444.5
Type: SR
# Max. Min./Amp. JD0 Period
12.535 r Y 0.145 r 2458316.07950 24.606285200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:00:22.12 +59:04:43.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:00:22.12 +59:04:43.1: 13.36 +/- 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 11.1958* 00 00 22.12 +59 04 43.1 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
ZTF J000022.06+590444.5,2461232.6958,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J000022.06+590444.5 20260711.1958 10.24CV 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 11.1958 2461232.6958 9.63 23:28:44.53 +52:55:57.7
110.52467 -7.93538 galactic Cas Second-epoch detections are separated by 1.1" and 3.3 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 J352.1850+52.9355 | 23:28:44.53 +52:55:57.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:44.53 +52:55:57.7: 11.23 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:44.53 +52:55:57.7: 11.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1958* 23 28 44.53 +52 55 57.7 9.6 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
ATO J352.1850+52.9355,2461232.6958,9.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.1850+52.9355 20260711.1958 9.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.18 23:57:55.76 +58:55:29.3
116.06235 -3.23141 galactic Cas Second-epoch detections are separated by 1.2" and 2.6 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 1999225848010851968 | 23:57:55.76 +58:55:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.035 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:55.76 +58:55:29.3: 12.83 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:55.76 +58:55:29.3: 12.93 +/- 0.23 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 11.1958* 23 57 55.76 +58 55 29.3 9.2 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 1999225848010851968,2461232.6958,9.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1999225848010851968 20260711.1958 9.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 9.89 23:28:35.38 +52:59:58.6
110.52414 -7.86463 galactic Cas Second-epoch detections are separated by 0.6" and 3.2 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 1992529890917147648 | 23:28:35.34 +52:59:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.702+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:35.38 +52:59:58.6: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:35.38 +52:59:58.6: 13.51 +/- 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 11.1958* 23 28 35.38 +52 59 58.6 9.9 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 1992529890917147648,2461232.6958,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992529890917147648 20260711.1958 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.62 23:59:50.44 +58:09:38.2
116.15181 -4.03029 galactic Cas Second-epoch detections are separated by 1.4" and 2.9 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 | 23:59:50.44 +58:09:38.2 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.038 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:50.44 +58:09:38.2: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:50.44 +58:09:38.2: 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 11.1958* 23 59 50.44 +58 09 38.2 10.6 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,2461232.6958,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.29 23:58:33.85 +58:47:50.2
116.11662 -3.37306 galactic Cas Second-epoch detections are separated by 0.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:33.85 +58:47:50.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.359+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:33.85 +58:47:50.2: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:33.85 +58:47:50.2: 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 11.1958* 23 58 33.85 +58 47 50.2 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461232.6958,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1958 2461232.6958 10.18 23:59:43.96 +59:01:09.6
116.30947 -3.18598 galactic Cas Second-epoch detections are separated by 0.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:59:43.96 +59:01:09.6 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:43.96 +59:01:09.6: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:43.96 +59:01:09.6: 13.40 +/- 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 11.1958* 23 59 43.96 +59 01 09.6 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
target,2461232.6958,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1958 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461232.69602170 11.07.2026 04:42:06.275 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.84
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: 7 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): 21902
Objects passed selection criteria: 21792
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 13242.8
Average stars matched: 12832.8 (96.904 %)
Memory usage VmPeak: 126212 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 10 19:09:57 CDT 2026
VaST build number 1.0rc89-143-g13f85f26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 11 01:11:21 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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461232.69602170 11.07.2026 04:42:06.275 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 218
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
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: 44 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): 151151
Objects passed selection criteria: 150562
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 95133.8
Average stars matched: 91167.5 (95.8309 %)
Memory usage VmPeak: 1979180 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 10 19:09:57 CDT 2026
VaST build number 1.0rc89-143-g13f85f26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 11 01:17:11 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
SExtractor catalog cache: saved Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.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: 2461232.69549681
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits exists and is non-empty
Saving wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits to local_wcs_cache/
'wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'local_wcs_cache/wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits exists and is non-empty
Saving wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits to local_wcs_cache/
'wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'local_wcs_cache/wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits'
wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
Image size: 942.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:53.114 +54:02:17.35 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 23:59:53.114 +54:02:17.35
Angular distance between the image centers 0.0377 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
Image size: 942.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:51.062 +54:02:20.26 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 23:59:51.062 +54:02:20.26
Angular distance between the image centers 0.0413 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:53.114 +54:02:17.35
Second-epoch second image center 23:59:51.062 +54:02:20.26
Angular distance between the image centers 0.00509 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits &> /tmp/tmp.deV1n5JD9o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits &> /tmp/tmp.WlNs1FwiiT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits &> /tmp/tmp.sjqj6Hq9lR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits &> /tmp/tmp.b41Vk52uMI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q1b1x1_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 22.497200
a=0.000000 b=1.000000 c=22.497200
From vast_summary.log: estimated ref. image limiting mag.: -7.84
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.66
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.66
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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (aperture=6.5)
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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
3.6 pix fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
3.5 pix fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
2.3 pix wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Limiting magnitude estimates:
14.7 mag. Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
14.7 mag. Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
12.5 mag. fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
12.5 mag. fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 10.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.deV1n5JD9o (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1910, bad_region=0, passed=23386
Got 23386 stars (including 21456 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_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 345 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 237 matched stars entering correct_measured_positions(), 165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 5401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.13"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0050 through 0 to 14.8900, gap 14.8900 to 345.0050
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 391 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 311 matched stars entering correct_measured_positions(), 5436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.00"
Accuracy estimation diagnostic: 307 matched stars entering correct_measured_positions(), 6969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.20"
Excluding outliers - 307 stars left (next iteration limit 248)
WCS_QUALITY_DIAG: file=Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits N_match=307 sigma_overall_arcsec=9.990 sigma_q1_arcsec=26.120 sigma_q2_arcsec=23.868 sigma_q3_arcsec=5.575 sigma_q4_arcsec=9.476 n_q1=31 n_q2=24 n_q3=81 n_q4=171 worst_quadrant_to_overall_ratio=2.615
The image catalog is written to wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -region wcs_Cas-04-Q1b1x1_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-Q1b1x1_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.WlNs1FwiiT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1872, bad_region=0, passed=23366
Got 23366 stars (including 21472 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_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 349 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(), 166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.90"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 228 matched stars entering correct_measured_positions(), 5186 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.88"
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 345.0155 through 0 to 14.8915, gap 14.8915 to 345.0155
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 391 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 316 matched stars entering correct_measured_positions(), 5214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.84"
Accuracy estimation diagnostic: 313 matched stars entering correct_measured_positions(), 6885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.49"
Excluding outliers - 313 stars left (next iteration limit 250)
WCS_QUALITY_DIAG: file=Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits N_match=313 sigma_overall_arcsec=12.138 sigma_q1_arcsec=31.673 sigma_q2_arcsec=30.888 sigma_q3_arcsec=5.656 sigma_q4_arcsec=10.621 n_q1=29 n_q2=29 n_q3=87 n_q4=168 worst_quadrant_to_overall_ratio=2.609
The image catalog is written to wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -region wcs_Cas-04-Q1b1x1_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-Q1b1x1_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.sjqj6Hq9lR (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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=73, bad_region=0, passed=2882
Got 2882 stars (including 2808 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat
util/solve_plate_with_UCAC5 got 2882 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4612 through 0 to 15.2187, gap 15.2187 to 345.4612
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 2753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4611 through 0 to 15.2181, gap 15.2181 to 345.4611
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 2751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 2751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits N_match=950 sigma_overall_arcsec=0.545 sigma_q1_arcsec=0.499 sigma_q2_arcsec=0.675 sigma_q3_arcsec=0.456 sigma_q4_arcsec=0.467 n_q1=176 n_q2=316 n_q3=153 n_q4=305 worst_quadrant_to_overall_ratio=1.239
The image catalog is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits -region wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.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.b41Vk52uMI (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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=99, bad_region=0, passed=3634
Got 3634 stars (including 3532 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
util/solve_plate_with_UCAC5 got 3634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3943 through 0 to 15.1814, gap 15.1814 to 345.3943
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 3457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3941 through 0 to 15.1802, gap 15.1802 to 345.3941
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 3457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 3457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits N_match=942 sigma_overall_arcsec=0.542 sigma_q1_arcsec=0.600 sigma_q2_arcsec=0.602 sigma_q3_arcsec=0.469 sigma_q4_arcsec=0.551 n_q1=149 n_q2=286 n_q3=179 n_q4=328 worst_quadrant_to_overall_ratio=1.110
The image catalog is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits -region wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits sigma_overall=9.990 worst_q_ratio=2.615
ref2=Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits sigma_overall=12.138 worst_q_ratio=2.609
new1=fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits sigma_overall=0.545 worst_q_ratio=1.239
new2=fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits sigma_overall=0.542 worst_q_ratio=1.110
reference average sigma_overall=11.064 worst_q_ratio=2.612
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006_astrometric_residuals.png (307 matched stars from wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 6.11 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007_astrometric_residuals.png (313 matched stars from wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 5.59 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120_astrometric_residuals.png (950 matched stars from wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121_astrometric_residuals.png (942 matched stars from wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits'
Preparing the HTML report for the field Cas-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31428_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31428_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:59.19 +49:04:15.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31433_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31433_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:36:15.03 +48:33:14.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31446_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31446_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:47:28.04 +50:24:35.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31459_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31459_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:39:36.71 +48:27:50.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31463_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31463_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:46:55.67 +50:17:22.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31464_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31464_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:46:46.36 +50:16:11.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31470_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31470_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:24.55 +49:35:30.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31474_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31474_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:41:40.37 +48:27:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31487_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31487_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:46:23.33 +50:04:35.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31488_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31488_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:42:45.71 +49:22:27.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31509_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 31509_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:45:11.50 +49:53:07.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05724_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 05724_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:09:36.48 +51:34:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20884_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 20884_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:36:01.27 +57:54:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17518_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 17518_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:40:30.29 +56:32:11.1 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cas-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
SExtractor catalog cache: saved Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits exists and is non-empty
wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits exists and is non-empty
wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits exists and is non-empty
wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
Image size: 942.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:53.114 +54:02:17.35 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 23:59:53.114 +54:02:17.35
Angular distance between the image centers 0.0377 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
Image size: 942.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:51.062 +54:02:20.26 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 23:59:51.062 +54:02:20.26
Angular distance between the image centers 0.0413 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:53.114 +54:02:17.35
Second-epoch second image center 23:59:51.062 +54:02:20.26
Angular distance between the image centers 0.00509 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits &> /tmp/tmp.wYyA1yXSXJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits &> /tmp/tmp.kXf36XSOjK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits &> /tmp/tmp.GNJJK4j9vO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits &> /tmp/tmp.Tn3sm78GPr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q1b1x1_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 20.732500
a=0.000000 b=1.000000 c=20.732500
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.21
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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (aperture=4.9)
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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 164 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.2 pix Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
3.4 pix fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
3.2 pix fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
2.1 pix wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.2 pix wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Limiting magnitude estimates:
13.2 mag. Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
13.2 mag. Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
11.1 mag. fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
11.1 mag. fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
All-image limiting magnitude estimate: 11.1 (SNR ) 10.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wYyA1yXSXJ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=63, blended=20826, bad_region=0, passed=167219
Got 167219 stars (including 146233 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 167219 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: 222 matched stars entering correct_measured_positions(), 146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 208 matched stars entering correct_measured_positions(), 33653 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.71"
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 344.9694 through 0 to 14.9892, gap 14.9892 to 344.9694
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 360 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 292 matched stars entering correct_measured_positions(), 33677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.71"
Accuracy estimation diagnostic: 290 matched stars entering correct_measured_positions(), 48882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.93"
Excluding outliers - 290 stars left (next iteration limit 228)
WCS_QUALITY_DIAG: file=Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits N_match=290 sigma_overall_arcsec=11.399 sigma_q1_arcsec=29.527 sigma_q2_arcsec=27.493 sigma_q3_arcsec=8.498 sigma_q4_arcsec=9.739 n_q1=35 n_q2=26 n_q3=75 n_q4=154 worst_quadrant_to_overall_ratio=2.590
The image catalog is written to wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -region wcs_Cas-04-Q1b1x1_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-Q1b1x1_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.kXf36XSOjK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=63, blended=20515, bad_region=0, passed=165641
Got 165641 stars (including 144957 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 165641 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 324 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 229 matched stars entering correct_measured_positions(), 153 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.03"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 217 matched stars entering correct_measured_positions(), 34789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.82"
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 344.9606 through 0 to 14.9544, gap 14.9544 to 344.9606
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 372 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 307 matched stars entering correct_measured_positions(), 34836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.81"
Accuracy estimation diagnostic: 303 matched stars entering correct_measured_positions(), 50288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.83"
Excluding outliers - 303 stars left (next iteration limit 238)
WCS_QUALITY_DIAG: file=Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits N_match=303 sigma_overall_arcsec=12.967 sigma_q1_arcsec=26.369 sigma_q2_arcsec=28.802 sigma_q3_arcsec=8.607 sigma_q4_arcsec=11.479 n_q1=34 n_q2=23 n_q3=87 n_q4=159 worst_quadrant_to_overall_ratio=2.221
The image catalog is written to wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -region wcs_Cas-04-Q1b1x1_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-Q1b1x1_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.GNJJK4j9vO (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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=767, bad_region=1, passed=22114
Got 22114 stars (including 21315 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat
util/solve_plate_with_UCAC5 got 22114 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3941 through 0 to 15.3367, gap 15.3367 to 345.3941
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 20942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3939 through 0 to 15.3358, gap 15.3358 to 345.3939
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 20941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 20941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits N_match=948 sigma_overall_arcsec=0.560 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.678 sigma_q3_arcsec=0.499 sigma_q4_arcsec=0.499 n_q1=176 n_q2=298 n_q3=153 n_q4=321 worst_quadrant_to_overall_ratio=1.211
The image catalog is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits -region wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.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.Tn3sm78GPr (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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1024, bad_region=1, passed=27752
Got 27752 stars (including 26683 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
util/solve_plate_with_UCAC5 got 27752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.2972 through 0 to 15.3365, gap 15.3365 to 345.2972
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 26338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.2970 through 0 to 15.3354, gap 15.3354 to 345.2970
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 26339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 26339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits N_match=943 sigma_overall_arcsec=0.557 sigma_q1_arcsec=0.608 sigma_q2_arcsec=0.619 sigma_q3_arcsec=0.450 sigma_q4_arcsec=0.535 n_q1=144 n_q2=276 n_q3=183 n_q4=340 worst_quadrant_to_overall_ratio=1.112
The image catalog is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits -region wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.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-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-41-20_20.00sec_0.00C_LIGHTs_0120.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.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_2026-07-10_CI_Cas-04-Q1b1x1_234922_TTUQ1b1x1_721601_h1sdNUFi/wcs_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121.fits
Preparing the HTML report for the field Cas-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:13.23 +50:39:03.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:45.10 +58:10:06.7: 11.90 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:53:07.33 +54:59:08.3: 12.52 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:10.24 +55:54:23.5: 10.88 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:53:15.27 +50:38:28.6: 12.70 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:10.24 +55:54:23.5: 10.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.74 +/- 0.02
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:13.23 +50:39:03.9: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:45.10 +58:10:06.7: 11.37 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 00:48:10.24 +55:54:23.5: ref_mag=10.74 +/- 0.02 new_mean_mag=10.1627 delta=0.58 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:53:07.33 +54:59:08.3: 12.13 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:53:15.27 +50:38:28.6: 12.51 +/- 0.13 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.06
Forced photometry reference-image weighted average: 12.31 +/- 0.10
Forced photometry filter KEPT candidate at 00:46:45.10 +58:10:06.7: ref_mag=11.58 +/- 0.06 new_mean_mag=10.1551 delta=1.43 (need > 0.90)
Forced photometry reference-image weighted average: 12.61 +/- 0.09
Forced photometry filter KEPT candidate at 00:53:07.33 +54:59:08.3: ref_mag=12.31 +/- 0.10 new_mean_mag=9.8834 delta=2.43 (need > 0.90)
Forced photometry filter KEPT candidate at 23:53:15.27 +50:38:28.6: ref_mag=12.61 +/- 0.09 new_mean_mag=9.7397 delta=2.87 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:57:24.05 +57:00:14.0: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:57:24.05 +57:00:14.0: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:15.37 +48:36:45.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:15.37 +48:36:45.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 00:33:15.37 +48:36:45.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:23.41 +48:47:52.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:51:01.34 +54:24:58.9: 9.02 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:51:01.34 +54:24:58.9: 8.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 8.88 +/- 0.00
Forced photometry filter REJECTED candidate at 00:51:01.34 +54:24:58.9: ref_mag=8.88 +/- 0.00 new_mean_mag=9.5836 delta=-0.70 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:23.41 +48:47:52.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:34.65 +48:54:32.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:34.65 +48:54:32.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:56:51.93 +57:23:42.4: 11.62 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:56:51.93 +57:23:42.4: 11.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.05
Forced photometry filter KEPT candidate at 00:56:51.93 +57:23:42.4: ref_mag=11.36 +/- 0.05 new_mean_mag=10.0041 delta=1.36 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:01.07 +48:38:59.6: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:01.07 +48:38:59.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:23.37 +50:31:39.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:23.37 +50:31:39.3: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:32.88 +48:52:56.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:32.88 +48:52:56.4: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:25.41 +57:41:21.0: 13.15 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:25.41 +57:41:21.0: 12.77 +/- 0.20 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.15
Forced photometry filter KEPT candidate at 23:59:25.41 +57:41:21.0: ref_mag=12.93 +/- 0.15 new_mean_mag=10.5814 delta=2.35 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:05:07.08 +59:04:42.3: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:18:13.02 +51:33:59.2: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:05:07.08 +59:04:42.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:18:13.02 +51:33:59.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:33.06 +58:30:07.0: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:15.29 +53:00:21.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:33.06 +58:30:07.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:15.29 +53:00:21.8: 13.46 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.34
Forced photometry filter KEPT candidate at 23:29:15.29 +53:00:21.8: ref_mag=13.46 +/- 0.34 new_mean_mag=10.5440 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:09.90 +52:46:46.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:09.90 +52:46:46.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:17.33 +52:53:23.5: 13.02 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:17.33 +52:53:23.5: 13.17 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.16
Forced photometry filter KEPT candidate at 23:28:17.33 +52:53:23.5: ref_mag=13.06 +/- 0.16 new_mean_mag=10.5612 delta=2.50 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:56:50.84 +58:46:38.8: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:56:50.84 +58:46:38.8: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:45.64 +58:13:24.7: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:45.64 +58:13:24.7: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:45.25 +58:31:38.5: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:45.25 +58:31:38.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:56.96 +58:50:00.9: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:56.96 +58:50:00.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:59.33 +58:54:44.1: 13.11 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:59.33 +58:54:44.1: 13.41 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.11 +/- 0.21
Forced photometry filter KEPT candidate at 23:57:59.33 +58:54:44.1: ref_mag=13.11 +/- 0.21 new_mean_mag=9.1147 delta=4.00 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:40.44 +58:21:10.3: 12.82 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:40.44 +58:21:10.3: 12.40 +/- 0.15 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.11
Forced photometry filter KEPT candidate at 23:58:40.44 +58:21:10.3: ref_mag=12.59 +/- 0.11 new_mean_mag=9.3466 delta=3.24 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:03.21 +58:55:46.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:03.21 +58:55:46.3: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:10.70 +53:03:34.8: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:56:44.76 +58:48:59.3: 12.19 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:10.70 +53:03:34.8: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:56:44.76 +58:48:59.3: 11.84 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.06
Forced photometry filter KEPT candidate at 23:56:44.76 +58:48:59.3: ref_mag=12.01 +/- 0.06 new_mean_mag=8.8463 delta=3.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:48.93 +53:06:42.1: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:48.93 +53:06:42.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:11.05 +58:57:41.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:11.05 +58:57:41.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:07:35.41 +54:21:27.8: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:07:35.41 +54:21:27.8: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:31.98 +59:00:19.1: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:31.98 +59:00:19.1: 13.40 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.33
Forced photometry filter KEPT candidate at 23:58:31.98 +59:00:19.1: ref_mag=13.40 +/- 0.33 new_mean_mag=9.3979 delta=4.00 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:57.10 +53:04:00.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:57.10 +53:04:00.0: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:06.83 +58:53:50.9: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:06.83 +58:53:50.9: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:23.43 +58:53:22.8: 13.52 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:23.43 +58:53:22.8: 13.49 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.52 +/- 0.28
Forced photometry filter KEPT candidate at 23:58:23.43 +58:53:22.8: ref_mag=13.52 +/- 0.28 new_mean_mag=9.8152 delta=3.70 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:18.28 +59:01:10.2: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:18.28 +59:01:10.2: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:19.21 +58:18:04.8: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:19.21 +58:18:04.8: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:56.61 +58:49:24.5: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:56.61 +58:49:24.5: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:57.33 +58:59:11.1: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:57.33 +58:59:11.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:44.20 +58:54:10.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:44.20 +58:54:10.6: 13.32 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.34
Forced photometry filter KEPT candidate at 23:57:44.20 +58:54:10.6: ref_mag=13.32 +/- 0.34 new_mean_mag=9.4453 delta=3.88 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:04.28 +59:00:23.5: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:04.28 +59:00:23.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:38.70 +58:17:04.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:38.70 +58:17:04.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:14.26 +58:40:19.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:14.26 +58:40:19.1: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:56.07 +52:50:39.8: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:09.54 +58:55:51.4: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:56.07 +52:50:39.8: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:09.54 +58:55:51.4: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:11.84 +58:16:00.5: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:11.84 +58:16:00.5: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:33.79 +58:57:20.5: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:33.79 +58:57:20.5: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:07.43 +52:44:24.5: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:07.43 +52:44:24.5: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:00:13.60 +59:04:12.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:06.93 +58:59:45.4: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:00:13.60 +59:04:12.5: 13.30 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.33
Forced photometry filter KEPT candidate at 00:00:13.60 +59:04:12.5: ref_mag=13.30 +/- 0.33 new_mean_mag=9.7171 delta=3.59 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:06.93 +58:59:45.4: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:03.34 +52:46:31.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:03.34 +52:46:31.9: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:04.26 +59:01:35.4: 13.16 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:04.26 +59:01:35.4: 12.64 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.13
Forced photometry filter KEPT candidate at 23:58:04.26 +59:01:35.4: ref_mag=12.85 +/- 0.13 new_mean_mag=10.6710 delta=2.18 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:30.65 +59:01:43.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:30.65 +59:01:43.7: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:38.04 +52:52:58.2: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:02.71 +52:51:28.6: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:38.04 +52:52:58.2: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:02.71 +52:51:28.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:18.68 +58:30:47.8: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:18.68 +58:30:47.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:31.32 +58:56:22.5: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:31.32 +58:56:22.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:45.77 +58:45:41.4: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:26.31 +58:59:27.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:45.77 +58:45:41.4: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:26.31 +58:59:27.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:19.41 +58:22:25.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:19.41 +58:22:25.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:35.58 +53:06:43.8: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:35.58 +53:06:43.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:14.41 +52:57:59.6: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:31.80 +58:55:54.6: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:14.41 +52:57:59.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:31.80 +58:55:54.6: 13.22 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.28
Forced photometry filter KEPT candidate at 23:58:31.80 +58:55:54.6: ref_mag=13.22 +/- 0.28 new_mean_mag=10.1359 delta=3.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:54.38 +52:54:18.8: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:54.38 +52:54:18.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:37.32 +59:04:45.3: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:20.45 +59:00:01.9: 13.49 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:37.32 +59:04:45.3: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:20.45 +59:00:01.9: 13.39 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.21
Forced photometry filter KEPT candidate at 23:58:20.45 +59:00:01.9: ref_mag=13.45 +/- 0.21 new_mean_mag=9.2262 delta=4.22 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:49:29.57 +52:12:07.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:49:29.57 +52:12:07.4: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:12.86 +58:41:57.9: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:12.86 +58:41:57.9: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:56.63 +52:49:22.8: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:56.63 +52:49:22.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:00:22.12 +59:04:43.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:00:22.12 +59:04:43.1: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:44.53 +52:55:57.7: 11.23 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:44.53 +52:55:57.7: 11.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.03
Forced photometry filter KEPT candidate at 23:28:44.53 +52:55:57.7: ref_mag=11.13 +/- 0.03 new_mean_mag=9.6192 delta=1.51 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:55.76 +58:55:29.3: 12.83 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:55.76 +58:55:29.3: 12.93 +/- 0.23 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.14
Forced photometry filter KEPT candidate at 23:57:55.76 +58:55:29.3: ref_mag=12.87 +/- 0.14 new_mean_mag=9.1725 delta=3.69 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:35.38 +52:59:58.6: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:50.44 +58:09:38.2: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:35.38 +52:59:58.6: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:50.44 +58:09:38.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:33.85 +58:47:50.2: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:33.85 +58:47:50.2: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:43.96 +59:01:09.6: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:24.42 +52:53:21.5: 10.99 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:43.96 +59:01:09.6: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:24.42 +52:53:21.5: 10.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.80 +/- 0.02
Forced photometry filter REJECTED candidate at 23:28:24.42 +52:53:21.5: ref_mag=10.80 +/- 0.02 new_mean_mag=10.1279 delta=0.67 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out191981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out117437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98921.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 103s
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: 40s
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Considering the candidate 191631_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191631_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:54:30.33 +55:45:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191641_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 191641_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 191642_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191642_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
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Considering the candidate 191645_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 191645_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 191647_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 191647_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 191653_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191653_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:59.19 +49:04:15.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191659_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191659_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:36:15.05 +48:33:14.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191661_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191661_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:26.81 +49:53:40.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191667_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 191667_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 191675_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191675_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:47:28.16 +50:24:34.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191689_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191689_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:39:36.75 +48:27:51.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191690_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191690_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:46:55.79 +50:17:21.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191694_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191694_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:46:46.43 +50:16:11.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191700_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191700_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:24.52 +49:35:31.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191702_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191702_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:41:40.21 +48:27:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191706_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191706_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 191707_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 191707_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 191709_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191709_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 191716_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191716_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:42:39.85 +49:34:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191719_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191719_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:46:23.39 +50:04:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191722_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191722_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:44:20.06 +49:36:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191726_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191726_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:42:45.65 +49:22:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191727_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191727_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 191733_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191733_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:42:51.19 +49:49:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191736_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191736_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 191751_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191751_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:42:22.53 +49:20:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191752_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191752_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:45:11.50 +49:53:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191754_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191754_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 191755_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191755_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:44:04.63 +49:04:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191777_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191777_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
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Considering the candidate 191800_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191800_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:39:11.38 +49:08:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191803_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191803_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:46:23.76 +49:40:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191806_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191806_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 191825_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191825_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:44:18.33 +49:41:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191841_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191841_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:39:45.56 +48:49:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191846_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191846_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 191849_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191849_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 191854_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191854_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:45:03.87 +50:08:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191862_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191862_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 191869_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191869_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:45:59.18 +49:31:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191889_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191889_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:44:43.55 +49:56:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191891_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191891_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:40:24.58 +49:11:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191894_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191894_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:44:42.46 +48:36:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191915_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191915_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:48:41.42 +57:48:14.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 191917_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191917_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:40.73 +49:06:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191925_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191925_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:41:13.53 +49:05:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191929_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 191929_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 191953_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191953_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
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Considering the candidate 191955_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191955_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:45:07.05 +50:08:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191964_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191964_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:57.94 +49:10:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191969_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191969_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:21.63 +49:38:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191971_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191971_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 191974_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191974_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:24.21 +50:02:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191981_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191981_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:39:34.65 +48:54:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.70, MAG_FAINT_SEARCH_LIMIT=10.68)GAIADR2_OUTPUT=# 2.138 390640023034538624 009.89354678972 +48.90926548139 10.6490 10.1962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 191984_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191984_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 191987_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 191987_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:38.31 +49:20:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192000_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192000_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:55:01.10 +57:15:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192003_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192003_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:47:03.40 +50:06:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192008_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192008_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:42:44.20 +49:19:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192009_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192009_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:54:57.74 +57:50:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192013_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192013_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:45:24.35 +49:51:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192017_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 192017_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 192029_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192029_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:45:47.84 +50:18:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192031_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192031_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:41:17.24 +49:10:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192032_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192032_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 192041_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192041_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:44:45.75 +49:11:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192046_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192046_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:42:29.79 +48:44:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192056_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192056_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:46:32.47 +50:11:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192057_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192057_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:47:22.56 +50:18:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192063_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 192063_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 192064_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192064_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:52:23.67 +55:37:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192066_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192066_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:25.52 +48:32:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192069_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192069_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 192077_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192077_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 192093_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192093_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:41:45.73 +48:31:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192095_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192095_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:45:53.85 +49:17:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192104_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192104_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:42:50.93 +48:32:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192107_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192107_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:47:02.78 +50:09:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192109_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192109_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:44:26.46 +56:45:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192113_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 192113_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 192129_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192129_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 192139_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192139_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:44:01.18 +49:39:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192143_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192143_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 192162_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192162_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:42:18.59 +49:52:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192163_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192163_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:55.84 +49:36:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192165_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192165_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:41:20.61 +48:32:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192175_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192175_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:41:25.09 +49:05:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192183_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 192183_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 192231_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192231_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:44:43.51 +49:42:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192234_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 192234_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 192244_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192244_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:40:04.46 +49:06:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192246_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192246_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:43:53.56 +49:30:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192286_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 192286_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 152173_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152173_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 35830_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 35830_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 119617_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 119617_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 63623_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 63623_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 60391_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 60391_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 61933_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 61933_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 155379_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 155379_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 160670_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 160670_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 119462_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 119462_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 154897_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 154897_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 153150_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 153150_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 159223_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 159223_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 153562_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 153562_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 64604_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 64604_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 154759_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 154759_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 65583_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 65583_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 153466_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 153466_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 98921_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 98921_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 153017_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 153017_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 64825_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 64825_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 154195_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 154195_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 117854_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 117854_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 117437_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 117437_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 159993_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 159993_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 154212_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 154212_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
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Considering the candidate 152990_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152990_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153957_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 153957_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117449_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 117449_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120586_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 120586_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118730_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 118730_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60968_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 60968_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117690_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 117690_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120634_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 120634_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153692_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 153692_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158496_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 158496_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 23:58:36.12 +58:25:44.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59575_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 59575_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152683_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152683_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35911_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 35911_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:09:36.47 +51:34:01.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152896_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152896_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60159_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 60159_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152874_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152874_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152832_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152832_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61741_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 61741_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61224_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 61224_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157557_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 157557_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153504_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 153504_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118368_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 118368_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152721_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152721_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121238_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 121238_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:36:01.25 +57:54:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120200_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 120200_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65731_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 65731_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62907_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 62907_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153820_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 153820_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62070_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 62070_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152985_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152985_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153212_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 153212_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178367_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 178367_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156031_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 156031_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60757_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 60757_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152835_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152835_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62646_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 62646_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117694_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 117694_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158272_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 158272_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 23:57:21.26 +58:25:03.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63923_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 63923_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161269_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 161269_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154887_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 154887_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152973_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
Preparing report for the candidate 152973_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61883_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 61883_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164998_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 164998_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:40:30.14 +56:32:11.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81909_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 81909_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:36:57.84 +53:53:48.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120446_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121
The candidate 120446_fd_Cas-04-Q1b1x1_2026-07-10_23-42-06_20.00sec_-0.00C_LIGHTs_0121 did not pass the final checks
**** FOUND 00:49:09.60 +57:48:38.9 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 151s
Prepared the HTML report for the field Cas-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:59:18.28 +59:01:10.2
23:58:04.28 +59:00:23.5
23:59:09.54 +58:55:51.4
23:57:55.76 +58:55:29.3
23:58:23.43 +58:53:22.8
23:58:45.77 +58:45:41.4
23:58:14.26 +58:40:19.1
23:58:45.25 +58:31:38.5
23:58:33.06 +58:30:07.0
23:59:19.41 +58:22:25.9
23:58:38.70 +58:17:04.5
23:59:11.84 +58:16:00.5
00:05:07.08 +59:04:42.3
00:00:13.60 +59:04:12.5
23:59:26.31 +58:59:27.8
23:58:30.65 +59:01:43.7
00:00:22.12 +59:04:43.1
23:58:04.26 +59:01:35.4
23:59:06.93 +58:59:45.4
23:59:43.96 +59:01:09.6
23:58:37.32 +59:04:45.3
23:57:57.33 +58:59:11.1
23:58:31.98 +59:00:19.1
23:57:59.33 +58:54:44.1
23:58:20.45 +59:00:01.9
23:58:11.05 +58:57:41.5
00:07:31.32 +58:56:22.5
23:58:03.21 +58:55:46.3
23:58:33.79 +58:57:20.5
23:58:31.80 +58:55:54.6
23:57:44.20 +58:54:10.6
23:58:06.83 +58:53:50.9
23:57:56.61 +58:49:24.5
23:56:44.76 +58:48:59.3
23:58:33.85 +58:47:50.2
23:57:56.96 +58:50:00.9
23:56:50.84 +58:46:38.8
23:58:12.86 +58:41:57.9
23:57:18.68 +58:30:47.8
23:58:40.44 +58:21:10.3
23:59:19.21 +58:18:04.8
23:58:45.64 +58:13:24.7
23:59:50.44 +58:09:38.2
00:49:29.57 +52:12:07.4
00:46:45.10 +58:10:06.7
00:53:07.33 +54:59:08.3
23:53:15.27 +50:38:28.6
00:47:13.23 +50:39:03.9
00:57:24.05 +57:00:14.0
00:38:23.41 +48:47:52.8
00:56:51.93 +57:23:42.4
00:34:01.07 +48:38:59.6
23:59:23.37 +50:31:39.3
00:34:32.88 +48:52:56.4
23:59:25.41 +57:41:21.0
00:18:13.02 +51:33:59.2
23:28:07.43 +52:44:24.5
23:28:03.34 +52:46:31.9
23:28:09.90 +52:46:46.7
23:28:56.63 +52:49:22.8
23:28:56.07 +52:50:39.8
23:29:02.71 +52:51:28.6
23:28:38.04 +52:52:58.2
23:28:17.33 +52:53:23.5
23:28:54.38 +52:54:18.8
23:28:44.53 +52:55:57.7
23:29:14.41 +52:57:59.6
23:29:15.29 +53:00:21.8
23:28:35.38 +52:59:58.6
23:29:10.70 +53:03:34.8
23:28:57.10 +53:04:00.0
23:28:48.93 +53:06:42.1
23:28:35.58 +53:06:43.8
23:07:35.41 +54:21:27.8
########### Completed Cas-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
00:46:45.10 +58:10:06.7
00:53:07.33 +54:59:08.3
23:53:15.27 +50:38:28.6
00:47:13.23 +50:39:03.9
00:57:24.05 +57:00:14.0
00:38:23.41 +48:47:52.8
00:56:51.93 +57:23:42.4
00:34:01.07 +48:38:59.6
23:59:23.37 +50:31:39.3
00:34:32.88 +48:52:56.4
23:59:25.41 +57:41:21.0
00:05:07.08 +59:04:42.3
00:18:13.02 +51:33:59.2
23:58:33.06 +58:30:07.0
23:29:15.29 +53:00:21.8
23:28:09.90 +52:46:46.7
23:28:17.33 +52:53:23.5
23:56:50.84 +58:46:38.8
23:58:45.64 +58:13:24.7
23:58:45.25 +58:31:38.5
23:57:56.96 +58:50:00.9
23:57:59.33 +58:54:44.1
23:58:40.44 +58:21:10.3
23:58:03.21 +58:55:46.3
23:29:10.70 +53:03:34.8
23:56:44.76 +58:48:59.3
23:28:48.93 +53:06:42.1
23:58:11.05 +58:57:41.5
23:07:35.41 +54:21:27.8
23:58:31.98 +59:00:19.1
23:28:57.10 +53:04:00.0
23:58:06.83 +58:53:50.9
23:58:23.43 +58:53:22.8
23:59:18.28 +59:01:10.2
23:59:19.21 +58:18:04.8
23:57:56.61 +58:49:24.5
23:57:57.33 +58:59:11.1
23:57:44.20 +58:54:10.6
23:58:04.28 +59:00:23.5
23:58:38.70 +58:17:04.5
23:58:14.26 +58:40:19.1
23:28:56.07 +52:50:39.8
23:59:09.54 +58:55:51.4
23:59:11.84 +58:16:00.5
23:58:33.79 +58:57:20.5
23:28:07.43 +52:44:24.5
00:00:13.60 +59:04:12.5
23:59:06.93 +58:59:45.4
23:28:03.34 +52:46:31.9
23:58:04.26 +59:01:35.4
23:58:30.65 +59:01:43.7
23:28:38.04 +52:52:58.2
23:29:02.71 +52:51:28.6
23:57:18.68 +58:30:47.8
00:07:31.32 +58:56:22.5
23:58:45.77 +58:45:41.4
23:59:26.31 +58:59:27.8
23:59:19.41 +58:22:25.9
23:28:35.58 +53:06:43.8
23:29:14.41 +52:57:59.6
23:58:31.80 +58:55:54.6
23:28:54.38 +52:54:18.8
23:58:37.32 +59:04:45.3
23:58:20.45 +59:00:01.9
00:49:29.57 +52:12:07.4
23:58:12.86 +58:41:57.9
23:28:56.63 +52:49:22.8
00:00:22.12 +59:04:43.1
23:28:44.53 +52:55:57.7
23:57:55.76 +58:55:29.3
23:28:35.38 +52:59:58.6
23:59:50.44 +58:09:38.2
23:58:33.85 +58:47:50.2
23:59:43.96 +59:01:09.6
###################################################################################
00:46:45.10 +58:10:06.7 -- not an asteroid (will add it to exclusion list)
00:53:07.33 +54:59:08.3 -- not an asteroid (will add it to exclusion list)
23:53:15.27 +50:38:28.6 -- not an asteroid (will add it to exclusion list)
00:47:13.23 +50:39:03.9 -- not an asteroid (will add it to exclusion list)
00:57:24.05 +57:00:14.0 -- not an asteroid (will add it to exclusion list)
00:38:23.41 +48:47:52.8 -- not an asteroid (will add it to exclusion list)
00:56:51.93 +57:23:42.4 -- not an asteroid (will add it to exclusion list)
00:34:01.07 +48:38:59.6 -- not an asteroid (will add it to exclusion list)
23:59:23.37 +50:31:39.3 -- not an asteroid (will add it to exclusion list)
00:34:32.88 +48:52:56.4 -- not an asteroid (will add it to exclusion list)
23:59:25.41 +57:41:21.0 -- not an asteroid (will add it to exclusion list)
00:05:07.08 +59:04:42.3 -- not an asteroid (will add it to exclusion list)
00:18:13.02 +51:33:59.2 -- not an asteroid (will add it to exclusion list)
23:58:33.06 +58:30:07.0 -- not an asteroid (will add it to exclusion list)
23:29:15.29 +53:00:21.8 -- not an asteroid (will add it to exclusion list)
23:28:09.90 +52:46:46.7 -- not an asteroid (will add it to exclusion list)
23:28:17.33 +52:53:23.5 -- not an asteroid (will add it to exclusion list)
23:56:50.84 +58:46:38.8 -- not an asteroid (will add it to exclusion list)
23:58:45.64 +58:13:24.7 -- not an asteroid (will add it to exclusion list)
23:58:45.25 +58:31:38.5 -- not an asteroid (will add it to exclusion list)
23:57:56.96 +58:50:00.9 -- not an asteroid (will add it to exclusion list)
23:57:59.33 +58:54:44.1 -- not an asteroid (will add it to exclusion list)
23:58:40.44 +58:21:10.3 -- not an asteroid (will add it to exclusion list)
23:58:03.21 +58:55:46.3 -- not an asteroid (will add it to exclusion list)
23:29:10.70 +53:03:34.8 -- not an asteroid (will add it to exclusion list)
23:56:44.76 +58:48:59.3 -- not an asteroid (will add it to exclusion list)
23:28:48.93 +53:06:42.1 -- not an asteroid (will add it to exclusion list)
23:58:11.05 +58:57:41.5 -- not an asteroid (will add it to exclusion list)
23:07:35.41 +54:21:27.8 -- not an asteroid (will add it to exclusion list)
23:58:31.98 +59:00:19.1 -- not an asteroid (will add it to exclusion list)
23:28:57.10 +53:04:00.0 -- not an asteroid (will add it to exclusion list)
23:58:06.83 +58:53:50.9 -- not an asteroid (will add it to exclusion list)
23:58:23.43 +58:53:22.8 -- not an asteroid (will add it to exclusion list)
23:59:18.28 +59:01:10.2 -- not an asteroid (will add it to exclusion list)
23:59:19.21 +58:18:04.8 -- not an asteroid (will add it to exclusion list)
23:57:56.61 +58:49:24.5 -- not an asteroid (will add it to exclusion list)
23:57:57.33 +58:59:11.1 -- not an asteroid (will add it to exclusion list)
23:57:44.20 +58:54:10.6 -- not an asteroid (will add it to exclusion list)
23:58:04.28 +59:00:23.5 -- not an asteroid (will add it to exclusion list)
23:58:38.70 +58:17:04.5 -- not an asteroid (will add it to exclusion list)
23:58:14.26 +58:40:19.1 -- not an asteroid (will add it to exclusion list)
23:28:56.07 +52:50:39.8 -- not an asteroid (will add it to exclusion list)
23:59:09.54 +58:55:51.4 -- not an asteroid (will add it to exclusion list)
23:59:11.84 +58:16:00.5 -- not an asteroid (will add it to exclusion list)
23:58:33.79 +58:57:20.5 -- not an asteroid (will add it to exclusion list)
23:28:07.43 +52:44:24.5 -- not an asteroid (will add it to exclusion list)
00:00:13.60 +59:04:12.5 -- not an asteroid (will add it to exclusion list)
23:59:06.93 +58:59:45.4 -- not an asteroid (will add it to exclusion list)
23:28:03.34 +52:46:31.9 -- not an asteroid (will add it to exclusion list)
23:58:04.26 +59:01:35.4 -- not an asteroid (will add it to exclusion list)
23:58:30.65 +59:01:43.7 -- not an asteroid (will add it to exclusion list)
23:28:38.04 +52:52:58.2 -- not an asteroid (will add it to exclusion list)
23:29:02.71 +52:51:28.6 -- not an asteroid (will add it to exclusion list)
23:57:18.68 +58:30:47.8 -- not an asteroid (will add it to exclusion list)
00:07:31.32 +58:56:22.5 -- not an asteroid (will add it to exclusion list)
23:58:45.77 +58:45:41.4 -- not an asteroid (will add it to exclusion list)
23:59:26.31 +58:59:27.8 -- not an asteroid (will add it to exclusion list)
23:59:19.41 +58:22:25.9 -- not an asteroid (will add it to exclusion list)
23:28:35.58 +53:06:43.8 -- not an asteroid (will add it to exclusion list)
23:29:14.41 +52:57:59.6 -- not an asteroid (will add it to exclusion list)
23:58:31.80 +58:55:54.6 -- not an asteroid (will add it to exclusion list)
23:28:54.38 +52:54:18.8 -- not an asteroid (will add it to exclusion list)
23:58:37.32 +59:04:45.3 -- not an asteroid (will add it to exclusion list)
23:58:20.45 +59:00:01.9 -- not an asteroid (will add it to exclusion list)
00:49:29.57 +52:12:07.4 -- not an asteroid (will add it to exclusion list)
23:58:12.86 +58:41:57.9 -- not an asteroid (will add it to exclusion list)
23:28:56.63 +52:49:22.8 -- not an asteroid (will add it to exclusion list)
00:00:22.12 +59:04:43.1 -- not an asteroid (will add it to exclusion list)
23:28:44.53 +52:55:57.7 -- not an asteroid (will add it to exclusion list)
23:57:55.76 +58:55:29.3 -- not an asteroid (will add it to exclusion list)
23:28:35.38 +52:59:58.6 -- not an asteroid (will add it to exclusion list)
23:59:50.44 +58:09:38.2 -- not an asteroid (will add it to exclusion list)
23:58:33.85 +58:47:50.2 -- not an asteroid (will add it to exclusion list)
23:59:43.96 +59:01:09.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:13.60 +59:04:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:00:22.12 +59:04:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:07.08 +59:04:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:31.32 +58:56:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:13.02 +51:33:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:01.07 +48:38:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:32.88 +48:52:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:23.41 +48:47:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:45.10 +58:10:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:13.23 +50:39:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:29.57 +52:12:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:07.33 +54:59:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:51.93 +57:23:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:24.05 +57:00:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:35.41 +54:21:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:03.34 +52:46:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:07.43 +52:44:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:09.90 +52:46:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:17.33 +52:53:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:35.38 +52:59:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:35.58 +53:06:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:38.04 +52:52:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:44.53 +52:55:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:48.93 +53:06:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:54.38 +52:54:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:56.07 +52:50:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:56.63 +52:49:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:57.10 +53:04:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:02.71 +52:51:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:10.70 +53:03:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:14.41 +52:57:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:15.29 +53:00:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:15.27 +50:38:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:44.76 +58:48:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:50.84 +58:46:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:18.68 +58:30:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:44.20 +58:54:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:55.76 +58:55:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:56.61 +58:49:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:56.96 +58:50:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:57.33 +58:59:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:59.33 +58:54:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:03.21 +58:55:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:04.26 +59:01:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:04.28 +59:00:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:06.83 +58:53:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:11.05 +58:57:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:12.86 +58:41:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:14.26 +58:40:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:20.45 +59:00:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:23.43 +58:53:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:30.65 +59:01:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:31.80 +58:55:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:31.98 +59:00:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:33.06 +58:30:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:33.79 +58:57:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:33.85 +58:47:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:37.32 +59:04:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:38.70 +58:17:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:40.44 +58:21:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:45.25 +58:31:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:45.64 +58:13:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:45.77 +58:45:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:06.93 +58:59:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:09.54 +58:55:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:11.84 +58:16:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:18.28 +59:01:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:19.21 +58:18:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:19.41 +58:22:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:23.37 +50:31:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:25.41 +57:41:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:26.31 +58:59:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:43.96 +59:01:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:50.44 +58:09:38.2 -- 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)
00:00:13.60 +59:04:12.5 -- not a known variable star
00:00:22.12 +59:04:43.1 -- a known variable star
00:05:07.08 +59:04:42.3 -- a known variable star
00:07:31.32 +58:56:22.5 -- a known variable star
00:18:13.02 +51:33:59.2 -- a known variable star
00:34:01.07 +48:38:59.6 -- not a known variable star
00:34:32.88 +48:52:56.4 -- not a known variable star
00:38:23.41 +48:47:52.8 -- not a known variable star
00:46:45.10 +58:10:06.7 -- not a known variable star
00:47:13.23 +50:39:03.9 -- a known variable star
00:49:29.57 +52:12:07.4 -- not a known variable star
00:53:07.33 +54:59:08.3 -- a known variable star
00:56:51.93 +57:23:42.4 -- not a known variable star
00:57:24.05 +57:00:14.0 -- not a known variable star
23:07:35.41 +54:21:27.8 -- not a known variable star
23:28:03.34 +52:46:31.9 -- not a known variable star
23:28:07.43 +52:44:24.5 -- a known variable star
23:28:09.90 +52:46:46.7 -- not a known variable star
23:28:17.33 +52:53:23.5 -- not a known variable star
23:28:35.38 +52:59:58.6 -- not a known variable star
23:28:35.58 +53:06:43.8 -- a known variable star
23:28:38.04 +52:52:58.2 -- a known variable star
23:28:44.53 +52:55:57.7 -- not a known variable star
23:28:48.93 +53:06:42.1 -- not a known variable star
23:28:54.38 +52:54:18.8 -- not a known variable star
23:28:56.07 +52:50:39.8 -- not a known variable star
23:28:56.63 +52:49:22.8 -- not a known variable star
23:28:57.10 +53:04:00.0 -- not a known variable star
23:29:02.71 +52:51:28.6 -- not a known variable star
23:29:10.70 +53:03:34.8 -- not a known variable star
23:29:14.41 +52:57:59.6 -- not a known variable star
23:29:15.29 +53:00:21.8 -- not a known variable star
23:53:15.27 +50:38:28.6 -- a known variable star
23:56:44.76 +58:48:59.3 -- a known variable star
23:56:50.84 +58:46:38.8 -- not a known variable star
23:57:18.68 +58:30:47.8 -- not a known variable star
23:57:44.20 +58:54:10.6 -- not a known variable star
23:57:55.76 +58:55:29.3 -- not a known variable star
23:57:56.61 +58:49:24.5 -- not a known variable star
23:57:56.96 +58:50:00.9 -- not a known variable star
23:57:57.33 +58:59:11.1 -- not a known variable star
23:57:59.33 +58:54:44.1 -- not a known variable star
23:58:03.21 +58:55:46.3 -- not a known variable star
23:58:04.26 +59:01:35.4 -- not a known variable star
23:58:04.28 +59:00:23.5 -- not a known variable star
23:58:06.83 +58:53:50.9 -- not a known variable star
23:58:11.05 +58:57:41.5 -- not a known variable star
23:58:12.86 +58:41:57.9 -- not a known variable star
23:58:14.26 +58:40:19.1 -- not a known variable star
23:58:20.45 +59:00:01.9 -- not a known variable star
23:58:23.43 +58:53:22.8 -- not a known variable star
23:58:30.65 +59:01:43.7 -- not a known variable star
23:58:31.80 +58:55:54.6 -- not a known variable star
23:58:31.98 +59:00:19.1 -- not a known variable star
23:58:33.06 +58:30:07.0 -- not a known variable star
23:58:33.79 +58:57:20.5 -- not a known variable star
23:58:33.85 +58:47:50.2 -- not a known variable star
23:58:37.32 +59:04:45.3 -- not a known variable star
23:58:38.70 +58:17:04.5 -- a known variable star
23:58:40.44 +58:21:10.3 -- a known variable star
23:58:45.25 +58:31:38.5 -- not a known variable star
23:58:45.64 +58:13:24.7 -- not a known variable star
23:58:45.77 +58:45:41.4 -- not a known variable star
23:59:06.93 +58:59:45.4 -- not a known variable star
23:59:09.54 +58:55:51.4 -- not a known variable star
23:59:11.84 +58:16:00.5 -- not a known variable star
23:59:18.28 +59:01:10.2 -- not a known variable star
23:59:19.21 +58:18:04.8 -- not a known variable star
23:59:19.41 +58:22:25.9 -- a known variable star
23:59:23.37 +50:31:39.3 -- not a known variable star
23:59:25.41 +57:41:21.0 -- a known variable star
23:59:26.31 +58:59:27.8 -- not a known variable star
23:59:43.96 +59:01:09.6 -- not a known variable star
23:59:50.44 +58:09:38.2 -- not a known variable star
Found 59 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
74 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 74 (excluding asteroids and hot pixels, 59 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)2461232.69549681 -observatory V36
07:29:59.77 +17:06:26.7 Mercury (5.3mag)
10:15:10.64 +12:18:44.0 Venus (-4.1mag)
04:26:40.42 +21:31:28.8 Mars (1.3mag)
08:17:26.55 +20:09:03.8 Jupiter (-1.8mag)
00:55:56.34 +03:20:47.7 Saturn (0.7mag)
04:07:23.68 +20:45:29.5 Uranus (5.8mag)
00:17:01.21 +00:20:36.5 Neptune (7.7mag)
20:30:50.29 -23:18:22.9 Pluto (14.4mag)
04:01:44.02 +25:01:39.5 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Jul 11 01:11 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461232.69549681:
08:17:23.19 +20:09:15.9 Io (6.1mag)
08:17:37.97 +20:08:21.6 Europa (6.3mag)
08:17:42.22 +20:08:04.0 Ganymede (5.6mag)
08:17:49.89 +20:07:35.5 Callisto (6.8mag)
08:15:55.69 +19:53:34.5 Himalia (15.7mag)
08:17:30.58 +20:08:49.0 Thebe (16.6mag)
08:15:16.81 +19:57:52.1 Elara (17.6mag)
08:21:00.35 +20:02:46.7 Pasiphae (17.8mag)
08:22:21.51 +20:14:16.0 Carme (19.0mag)
00:55:48.91 +03:20:29.3 Titan (8.5mag)
00:55:54.28 +03:20:36.7 Rhea (9.8mag)
00:55:24.65 +03:19:46.9 Iapetus (11.2mag)
00:56:02.28 +03:21:12.3 Hyperion (14.5mag)
00:55:55.96 +03:17:54.1 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 11 01:11 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461232.69549681:
17:47:58.20 -32:49:57.9 JWST
18:05:32.30 +32:36:46.2 Chandra
08:50:58.76 -49:46:02.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 11 01:11 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461232.69549681 -observatory V36
02:37:28.18 +14:31:44.1 17.9mag P/1996 R2 (Lagerkvist)
18:17:17.56 -34:23:11.6 13.7mag P/2010 H2 (Vales)
06:26:31.12 -68:09:10.2 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:01:05.97 +32:27:40.6 17.6mag C/2017 K2 (PANSTARRS)
17:02:52.68 +16:02:37.3 18.0mag C/2021 G2 (ATLAS)
01:52:36.47 +09:53:14.2 15.4mag P/2021 N1 (ZTF)
22:59:01.71 +32:17:03.7 17.3mag C/2022 E2 (ATLAS)
06:13:21.75 +26:55:08.2 16.7mag C/2022 N2 (PANSTARRS)
09:56:14.90 +29:44:35.9 16.8mag C/2022 QE78 (ATLAS)
09:10:16.70 +05:00:56.3 17.8mag C/2022 R6 (PANSTARRS)
18:06:42.24 +21:15:43.3 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:30.10 -11:24:24.8 17.7mag P/2023 B1 (PANSTARRS)
21:48:13.59 +67:36:58.4 17.8mag C/2023 H5 (Lemmon)
16:29:13.17 -10:10:00.2 13.9mag C/2023 R1 (PANSTARRS)
08:02:06.45 +65:45:13.3 17.9mag C/2024 A1 (ATLAS)
07:33:55.21 +30:02:48.2 14.6mag C/2024 E1 (Wierzchos)
15:15:55.04 +15:21:03.8 17.6mag C/2024 G6 (ATLAS)
19:40:14.53 +39:33:31.3 13.8mag C/2024 J3 (ATLAS)
21:46:43.00 +46:07:50.2 17.8mag C/2024 R4 (PANSTARRS)
04:50:26.16 -13:45:26.0 15.7mag C/2024 T5 (ATLAS)
06:35:16.33 +28:55:45.1 18.0mag C/2025 J1 (Borisov)
07:14:55.90 -12:57:49.9 16.5mag C/2025 R3 (PANSTARRS)
09:57:03.96 +22:24:04.0 17.6mag C/2025 V2 (Rankin)
12:44:53.80 +03:54:07.6 17.1mag C/2025 Y1 (ATLAS)
16:49:34.47 +79:08:18.9 17.3mag C/2026 A2 (Bok)
02:47:10.63 +45:16:34.8 16.7mag C/2026 B2 (Sun-Gao)
11:26:02.69 +04:41:42.8 17.0mag A/2026 E1
21:20:22.87 -15:22:30.0 7.2mag 10P/Tempel
11:13:50.92 -01:55:22.9 16.1mag 29P/Schwassmann-Wachmann
04:01:23.35 +29:38:42.2 17.9mag 47P/Ashbrook-Jackson
10:09:50.28 +13:44:35.0 17.0mag 63P/Wild
00:48:43.97 -05:04:58.3 15.5mag 65P/Gunn
08:29:35.11 +34:10:43.7 18.0mag 76P/West-Kohoutek-Ikemura
04:29:26.29 +20:13:23.4 13.7mag 78P/Gehrels
02:23:42.31 +10:43:36.3 16.2mag 88P/Howell
06:38:02.70 +30:29:09.8 15.7mag 93P/Lovas
04:23:43.91 +31:09:33.1 16.8mag 114P/Wiseman-Skiff
08:10:45.27 +30:36:37.7 15.2mag 123P/West-Hartley
10:49:42.10 +00:50:36.0 16.8mag 124P/Mrkos
04:53:05.02 +20:50:14.9 16.2mag 128P/Shoemaker-Holt
05:37:50.83 +19:42:28.5 17.8mag 131P/Mueller
00:01:46.74 +02:58:07.2 17.9mag 139P/Vaisala-Oterma
07:16:40.91 +16:50:21.2 15.6mag 141P-D/Machholz
03:17:12.46 -21:02:05.1 15.4mag 161P/Hartley-IRAS
05:36:05.83 +34:07:54.7 15.3mag 162P/SidingSpring
19:02:21.74 +15:35:51.6 14.7mag 169P/NEAT
01:43:02.98 +07:41:40.0 17.7mag 220P/McNaught
16:35:51.18 -08:25:05.1 17.0mag 235P/LINEAR
08:47:03.88 +33:13:20.1 17.9mag 240P/NEAT
20:41:50.25 -49:45:22.8 17.8mag 259P/Garradd
02:01:39.84 +12:29:21.5 15.7mag 260P/McNaught
05:39:46.79 +36:54:41.4 17.4mag 295P/LINEAR
15:06:34.02 +05:58:56.4 17.6mag 391P/Kowalski
08:35:21.55 +19:38:33.9 17.9mag 450P/LONEOS
07:53:05.48 +39:08:46.9 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 11 01:11 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 11 01:11 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 11 01:11 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:53:51.251 -11:21:33.08 AT 2026syq 2026-06-27.41 23.2367
23:14:22.224 -08:09:18.54 AT 2026syp 2026-06-27.43 22.6416
20:24:01.601 -11:52:50.82 AT 2026syo 2026-06-27.32 21.3589
21:39:57.862 -12:34:45.50 AT 2026syn 2026-06-27.33 22.2061
20:18:53.855 -11:01:07.67 AT 2026sym 2026-06-27.32 21.9202
22:46:14.843 -01:56:26.82 AT 2026syl 2026-06-27.41 22.8651
19:56:23.612 -14:52:03.64 AT 2026syk 2026-06-27.29 22.298
21:24:30.981 -14:08:25.72 AT 2026syj 2026-06-27.33 22.4129
21:16:17.516 -11:29:42.28 AT 2026syi 2026-06-27.34 22.8522
21:23:58.485 -06:44:08.17 AT 2026syh 2026-06-27.33 21.9873
22:43:56.471 -07:01:02.12 AT 2026syg 2026-06-27.41 22.6378
22:44:27.893 -09:14:49.58 AT 2026syf 2026-06-27.41 22.7315
23:02:17.769 -08:54:25.49 AT 2026sye 2026-06-27.42 21.7254
20:14:56.619 -18:30:02.61 AT 2026syd 2026-06-27.29 22.2007
20:49:57.648 -11:42:25.46 AT 2026syc 2026-06-27.30 22.962
21:15:07.018 -10:44:08.34 AT 2026syb 2026-06-27.34 22.1382
21:45:53.908 -10:06:22.31 AT 2026sya 2026-06-27.33 22.2361
21:28:25.130 -19:21:16.37 AT 2026sxz 2026-06-27.33 22.3064
22:56:47.457 -11:33:53.05 AT 2026sxy 2026-06-27.41 22.3592
23:00:56.153 -09:26:33.73 AT 2026sxx 2026-06-27.42 22.4667
-rw-r--r-- 1 apache apache 30K Jul 11 01:11 tns_transients_list.txt
