This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m
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 17.1600 2461238.6600 12.66 00:09:24.01 +54:46:43.2
116.83985 -7.59508 galactic Cas Second-epoch detections are separated by 1.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:09:24.01 +54:46:43.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:24.01 +54:46:43.2: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:24.01 +54:46:43.2: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 09 24.01 +54 46 43.2 12.7 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,2461238.6600,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.66CV 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 17.1600 2461238.6600 12.10 00:19:34.69 +55:29:44.7
118.39511 -7.09510 galactic Cas Second-epoch detections are separated by 1.8" and 1.2 pix
The object was found in VSX15" Gaia DR3 421391443420216832
Type: ROT
# Max. Min./Amp. JD0 Period
14.000 G 14.030 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:34.69 +55:29:44.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:34.69 +55:29:44.7: 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 17.1600* 00 19 34.69 +55 29 44.7 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421391443420216832,2461238.6600,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421391443420216832 20260717.1600 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.31 23:54:10.44 +57:04:44.9
115.17997 -4.92823 galactic Cas Second-epoch detections are separated by 3.0" and 1.6 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 | 23:54:10.44 +57:04:44.9 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.440+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:10.44 +57:04:44.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:10.44 +57:04:44.9: 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 17.1600* 23 54 10.44 +57 04 44.9 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.22 00:04:11.10 +55:35:59.3
116.24483 -6.65723 galactic Cas Second-epoch detections are separated by 2.8" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:04:11.10 +55:35:59.3 (user input) | T | P | (position from user input) J-Ks=14.788+/- (unrealisitic color!)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:11.10 +55:35:59.3: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:11.10 +55:35:59.3: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 04 11.10 +55 35 59.3 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.22CV 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 17.1600 2461238.6600 12.16 23:44:33.06 +53:02:41.7
112.85887 -8.51368 galactic Cas Second-epoch detections are separated by 1.3" and 1.4 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 | 23:44:33.06 +53:02:41.7 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:33.06 +53:02:41.7: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:33.06 +53:02:41.7: 13.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 44 33.06 +53 02 41.7 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.16CV 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 17.1600 2461238.6600 12.10 00:01:47.52 +56:08:36.5
116.01591 -6.06018 galactic Cas Second-epoch detections are separated by 0.9" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:01:47.52 +56:08:36.5 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.075 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:47.52 +56:08:36.5: 13.49 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:47.52 +56:08:36.5: 13.06 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 17.1600* 00 01 47.52 +56 08 36.5 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.58 23:27:00.60 +53:39:35.5
110.51215 -7.16363 galactic Cas Second-epoch detections are separated by 6.8" and 2.1 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 | 23:27:00.60 +53:39:35.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:00.60 +53:39:35.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:00.60 +53:39:35.5: 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 17.1600* 23 27 00.60 +53 39 35.5 12.6 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,2461238.6600,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.45 23:43:43.11 +51:35:38.7
112.35087 -9.88103 galactic Cas Second-epoch detections are separated by 1.9" and 1.1 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 1944695431391876480 | 23:43:42.47 +51:36:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:43.11 +51:35:38.7: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:43.11 +51:35:38.7: 13.65 +/- 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 17.1600* 23 43 43.11 +51 35 38.7 12.4 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 1944695431391876480,2461238.6600,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944695431391876480 20260717.1600 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.96 00:05:06.39 +54:18:27.5
116.13897 -7.95190 galactic Cas Second-epoch detections are separated by 3.1" and 0.9 pix
The object was found in VSX21" Gaia DR3 420298253984619520
Type: RS
# Max. Min./Amp. JD0 Period
14.480 G 14.630 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:05:06.39 +54:18:27.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:05:06.39 +54:18:27.5: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 05 06.39 +54 18 27.5 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420298253984619520,2461238.6600,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420298253984619520 20260717.1600 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.04 00:23:01.45 +53:17:43.1
118.63621 -9.33929 galactic Cas Second-epoch detections are separated by 1.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:01.45 +53:17:43.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:01.45 +53:17:43.1: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:01.45 +53:17:43.1: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 23 01.45 +53 17 43.1 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.11 23:44:22.42 +54:06:37.2
113.11176 -7.47778 galactic Cas Second-epoch detections are separated by 1.5" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.0855+54.0999 | 23:44:22.42 +54:06:37.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.449+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:22.42 +54:06:37.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:22.42 +54:06:37.2: 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 17.1600* 23 44 22.42 +54 06 37.2 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.0855+54.0999,2461238.6600,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.0855+54.0999 20260717.1600 12.11CV 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 17.1600 2461238.6600 12.31 23:45:18.41 +55:48:26.7
113.68081 -5.87197 galactic Cas Second-epoch detections are separated by 2.1" and 1.4 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 | 23:45:18.41 +55:48:26.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:18.41 +55:48:26.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:18.41 +55:48:26.7: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 45 18.41 +55 48 26.7 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.05 00:04:07.72 +56:06:31.7
116.33097 -6.15542 galactic Cas Second-epoch detections are separated by 0.8" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.0225+56.1167 | 00:04:07.72 +56:06:31.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.318+/-0.035 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:07.72 +56:06:31.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:07.72 +56:06:31.7: 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 17.1600* 00 04 07.72 +56 06 31.7 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.0225+56.1167,2461238.6600,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.0225+56.1167 20260717.1600 12.05CV 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 17.1600 2461238.6600 11.69 00:26:43.25 +57:15:39.5
119.57950 -5.44980 galactic Cas Second-epoch detections are separated by 1.1" and 1.5 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 | 00:26:43.25 +57:15:39.5 (user input) | T | P | (position from user input) J-Ks=0.728+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:43.25 +57:15:39.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:43.25 +57:15:39.5: 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 17.1600* 00 26 43.25 +57 15 39.5 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.08 23:45:47.75 +57:16:15.6
114.11866 -4.47323 galactic Cas Second-epoch detections are separated by 0.4" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.4612+57.2675 | 23:45:47.75 +57:16:15.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.345+/-0.058 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:47.75 +57:16:15.6: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:47.75 +57:16:15.6: 13.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 45 47.75 +57 16 15.6 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.4612+57.2675,2461238.6600,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.4612+57.2675 20260717.1600 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.91 23:40:06.44 +54:53:06.6
112.71844 -6.56586 galactic Cas Second-epoch detections are separated by 1.6" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.0317+54.8719 | 23:40:05.61 +54:52:49.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:40:06.44 +54:53:06.6: 12.91 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:40:06.44 +54:53:06.6: 12.75 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 17.1600* 23 40 06.44 +54 53 06.6 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.0317+54.8719,2461238.6600,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.0317+54.8719 20260717.1600 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.02 23:39:18.26 +52:16:23.0
111.87346 -9.04308 galactic Cas Second-epoch detections are separated by 1.5" and 1.1 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 | 23:39:18.26 +52:16:23.0 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.031 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:18.26 +52:16:23.0: 13.25 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:18.26 +52:16:23.0: 13.23 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 39 18.26 +52 16 23.0 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.00 00:14:34.69 +54:09:02.7
117.49290 -8.33128 galactic Cas Second-epoch detections are separated by 3.3" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:14:34.69 +54:09:02.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:34.69 +54:09:02.7: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:34.69 +54:09:02.7: 13.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 14 34.69 +54 09 02.7 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.04 23:41:11.69 +57:06:26.0
113.47228 -4.46880 galactic Cas Second-epoch detections are separated by 3.0" and 1.5 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 J355.3012+57.1115 | 23:41:13.68 +57:05:58.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:11.69 +57:06:26.0: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:11.69 +57:06:26.0: 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 17.1600* 23 41 11.69 +57 06 26.0 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.3012+57.1115,2461238.6600,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.3012+57.1115 20260717.1600 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.96 23:42:48.94 +51:38:41.5
112.22736 -9.79496 galactic Cas Second-epoch detections are separated by 7.1" and 2.5 pix
The object was found in VSX12" Gaia DR3 1944698729926124800
Type: ROT
# Max. Min./Amp. JD0 Period
16.800 G 16.860 G K
ATTENTION: measured mag 11.96 is 4.8 mag brighter than the VSX record maximum brightness 16.80 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:48.94 +51:38:41.5: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:48.94 +51:38:41.5: 13.65 +/- 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 17.1600* 23 42 48.94 +51 38 41.5 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944698729926124800,2461238.6600,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944698729926124800 20260717.1600 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.66 00:25:31.28 +56:42:26.6
119.36123 -5.98457 galactic Cas Second-epoch detections are separated by 3.7" and 1.9 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 J006.3841+56.7078 | 00:25:31.28 +56:42:26.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:31.28 +56:42:26.6: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:31.28 +56:42:26.6: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 25 31.28 +56 42 26.6 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J006.3841+56.7078,2461238.6600,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.3841+56.7078 20260717.1600 11.66CV 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 17.1600 2461238.6600 11.88 23:23:51.26 +49:17:44.6
108.58124 -11.12011 galactic And Second-epoch detections are separated by 3.7" and 1.7 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 | 23:23:51.26 +49:17:44.6 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:51.26 +49:17:44.6: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:51.26 +49:17:44.6: 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 17.1600* 23 23 51.26 +49 17 44.6 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 11.88CV 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 17.1600 2461238.6600 12.08 00:17:02.06 +57:24:19.4
118.29225 -5.15611 galactic Cas Second-epoch detections are separated by 3.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:17:02.06 +57:24:19.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:17:02.06 +57:24:19.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:17:02.06 +57:24:19.4: 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 17.1600* 00 17 02.06 +57 24 19.4 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.82 00:15:18.03 +53:07:47.9
117.45258 -9.35688 galactic Cas Second-epoch detections are separated by 0.6" and 1.5 pix
The object was found in VSX18" Gaia DR3 419243891056810368
Type: ROT
# Max. Min./Amp. JD0 Period
12.930 G 13.020 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:18.03 +53:07:47.9: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:18.03 +53:07:47.9: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 15 18.03 +53 07 47.9 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419243891056810368,2461238.6600,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419243891056810368 20260717.1600 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.82 23:50:03.35 +50:48:21.6
113.12624 -10.89339 galactic Cas Second-epoch detections are separated by 1.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1943993874253244032 | 23:50:02.21 +50:49:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1927AnHar.100...33C HD 236225 J-Ks=0.352+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:03.35 +50:48:21.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:03.35 +50:48:21.6: 13.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 50 03.35 +50 48 21.6 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943993874253244032,2461238.6600,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943993874253244032 20260717.1600 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.95 23:21:10.53 +53:55:05.7
109.78064 -6.63272 galactic Cas Second-epoch detections are separated by 1.0" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.2971+53.9128 | 23:21:10.67 +53:55:28.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.292+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:10.53 +53:55:05.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:10.53 +53:55:05.7: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 21 10.53 +53 55 05.7 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.2971+53.9128,2461238.6600,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.2971+53.9128 20260717.1600 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.80 23:41:09.34 +52:19:40.5
112.16427 -9.06832 galactic Cas Second-epoch detections are separated by 2.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1992993128908886784 | 23:41:08.05 +52:19:17.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:09.34 +52:19:40.5: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:09.34 +52:19:40.5: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 41 09.34 +52 19 40.5 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992993128908886784,2461238.6600,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992993128908886784 20260717.1600 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.72 23:46:38.90 +53:36:25.0
113.30961 -8.05001 galactic Cas Second-epoch detections are separated by 1.1" and 1.2 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 1993497559929926016 | 23:46:37.87 +53:36:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.497+/-0.048 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:38.90 +53:36:25.0: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:38.90 +53:36:25.0: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 46 38.90 +53 36 25.0 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993497559929926016,2461238.6600,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993497559929926016 20260717.1600 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.65 00:31:00.11 +57:25:00.4
120.17116 -5.34538 galactic Cas Second-epoch detections are separated by 1.5" and 1.4 pix
The object was found in VSX 2" Gaia DR3 421839975445105536
Type: E
# Max. Min./Amp. JD0 Period
13.480 G 13.690 G 2.085110000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:00.11 +57:25:00.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:00.11 +57:25:00.4: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 31 00.11 +57 25 00.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421839975445105536,2461238.6600,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421839975445105536 20260717.1600 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.94 23:17:04.21 +54:39:05.3
109.47513 -5.73590 galactic Cas Second-epoch detections are separated by 2.4" and 0.8 pix
The object was found in VSX11" Gaia DR3 1996793934448061696
Type: ROT
# Max. Min./Amp. JD0 Period
13.510 G 13.550 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:04.21 +54:39:05.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:04.21 +54:39:05.3: 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 17.1600* 23 17 04.21 +54 39 05.3 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996793934448061696,2461238.6600,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996793934448061696 20260717.1600 11.94CV 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 17.1600 2461238.6600 11.50 23:57:18.96 +54:52:41.6
115.13490 -7.17211 galactic Cas Second-epoch detections are separated by 1.9" and 1.4 pix
The object was found in VSX10" LP Cas
Type: M
# Max. Min./Amp. JD0 Period
14.900 pg < 17.000 pg 2429143.00000 294.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:18.96 +54:52:41.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:18.96 +54:52:41.6: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 57 18.96 +54 52 41.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LP Cas,2461238.6600,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LP Cas 20260717.1600 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.81 23:38:57.63 +54:45:08.9
112.52170 -6.64771 galactic Cas Second-epoch detections are separated by 1.4" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J354.7399+54.7525 | 23:38:57.63 +54:45:08.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.482+/-0.036 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:38:57.63 +54:45:08.9: 13.12 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:38:57.63 +54:45:08.9: 13.55 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 17.1600* 23 38 57.63 +54 45 08.9 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.7399+54.7525,2461238.6600,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.7399+54.7525 20260717.1600 11.81CV 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 17.1600 2461238.6600 11.80 23:32:25.66 +51:54:37.0
110.74323 -9.08180 galactic Cas Second-epoch detections are separated by 1.3" and 1.2 pix
The object was found in VSX 1" Gaia DR3 1992931384459555584
Type: VAR
# Max. Min./Amp. JD0 Period
13.620 G 13.760 G 0.014758400000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:25.66 +51:54:37.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:25.66 +51:54:37.0: 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 17.1600* 23 32 25.66 +51 54 37.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992931384459555584,2461238.6600,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992931384459555584 20260717.1600 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.47 00:19:05.99 +56:05:26.7
118.40292 -6.49637 galactic Cas Second-epoch detections are separated by 1.3" and 1.2 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 J004.7658+56.1014 | 00:19:05.99 +56:05:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.764+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:05.99 +56:05:26.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:05.99 +56:05:26.7: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 19 05.99 +56 05 26.7 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J004.7658+56.1014,2461238.6600,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.7658+56.1014 20260717.1600 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.72 23:39:31.70 +55:18:15.4
112.75442 -6.14014 galactic Cas Second-epoch detections are separated by 1.4" and 1.0 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 | 23:39:31.70 +55:18:15.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.460+/-0.042 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:31.70 +55:18:15.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:31.70 +55:18:15.4: 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 17.1600* 23 39 31.70 +55 18 15.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.74 23:36:55.82 +54:03:11.7
112.03716 -7.23493 galactic Cas Second-epoch detections are separated by 0.5" and 1.0 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 | 23:36:55.82 +54:03:11.7 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:55.82 +54:03:11.7: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:55.82 +54:03:11.7: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 36 55.82 +54 03 11.7 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.42 00:25:59.36 +55:56:51.7
119.34963 -6.74695 galactic Cas Second-epoch detections are separated by 0.7" and 1.3 pix
The object was found in VSX19" Gaia DR3 421314202732088960
Type: ROT
# Max. Min./Amp. JD0 Period
16.600 G 16.660 G K
ATTENTION: measured mag 11.42 is 5.2 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-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:59.36 +55:56:51.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:59.36 +55:56:51.7: 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 17.1600* 00 25 59.36 +55 56 51.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421314202732088960,2461238.6600,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421314202732088960 20260717.1600 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.36 00:10:28.24 +51:50:29.5
116.51679 -10.51921 galactic Cas Second-epoch detections are separated by 0.3" and 1.5 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 | 00:10:28.24 +51:50:29.5 (user input) | T | P | (position from user input) J-Ks=0.454+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:28.24 +51:50:29.5: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:28.24 +51:50:29.5: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 10 28.24 +51 50 29.5 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.55 23:28:57.54 +51:01:11.3
109.94182 -9.75983 galactic Cas Second-epoch detections are separated by 1.1" and 1.1 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 | 23:28:57.54 +51:01:11.3 (user input) | T | P | (position from user input) J-Ks=0.660+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:57.54 +51:01:11.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:57.54 +51:01:11.3: 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 17.1600* 23 28 57.54 +51 01 11.3 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.57 23:41:28.17 +52:04:54.8
112.14346 -9.31816 galactic Cas Second-epoch detections are separated by 2.6" and 1.6 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 J355.3702+52.0801 | 23:41:28.17 +52:04:54.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:28.17 +52:04:54.8: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:28.17 +52:04:54.8: 13.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 41 28.17 +52 04 54.8 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.3702+52.0801,2461238.6600,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.3702+52.0801 20260717.1600 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.56 23:30:17.84 +54:52:52.7
111.35989 -6.15704 galactic Cas Second-epoch detections are separated by 0.3" and 1.0 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 1997418766292819200 | 23:30:15.81 +54:52:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.362+/- (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:17.84 +54:52:52.7: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:17.84 +54:52:52.7: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 30 17.84 +54 52 52.7 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997418766292819200,2461238.6600,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997418766292819200 20260717.1600 11.56CV 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 17.1600 2461238.6600 11.66 23:14:01.73 +55:14:39.2
109.28271 -5.02504 galactic Cas Second-epoch detections are separated by 0.9" and 0.8 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 1997069465189797120 | 23:14:05.04 +55:14:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.350+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:01.73 +55:14:39.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:01.73 +55:14:39.2: 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 17.1600* 23 14 01.73 +55 14 39.2 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997069465189797120,2461238.6600,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997069465189797120 20260717.1600 11.66CV 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 17.1600 2461238.6600 11.62 23:15:56.67 +52:27:19.8
108.52049 -7.72374 galactic And Second-epoch detections are separated by 0.8" and 1.2 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 J348.9641+52.4446 | 23:15:51.67 +52:27:25.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.849+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:56.67 +52:27:19.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:56.67 +52:27:19.8: 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 17.1600* 23 15 56.67 +52 27 19.8 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.9641+52.4446,2461238.6600,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.9641+52.4446 20260717.1600 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.64 23:14:53.64 +56:49:23.2
109.97578 -3.60030 galactic Cas Second-epoch detections are separated by 3.4" and 0.8 pix
The object was found in VSX12" Gaia DR3 2009268752861844224
Type: S
# Max. Min./Amp. JD0 Period
17.090 G 17.840 G K
ATTENTION: measured mag 11.64 is 5.4 mag brighter than the VSX record maximum brightness 17.09 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:53.64 +56:49:23.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:53.64 +56:49:23.2: 13.34 +/- 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 17.1600* 23 14 53.64 +56 49 23.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009268752861844224,2461238.6600,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009268752861844224 20260717.1600 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.67 23:18:18.47 +56:19:03.0
110.23392 -4.24091 galactic Cas Second-epoch detections are separated by 2.6" and 0.9 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 J349.5618+56.3050 | 23:18:18.91 +56:18:47.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.715+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:18.47 +56:19:03.0: 13.22 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:18.47 +56:19:03.0: 13.11 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 17.1600* 23 18 18.47 +56 19 03.0 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.5618+56.3050,2461238.6600,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.5618+56.3050 20260717.1600 11.67CV 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 17.1600 2461238.6600 11.10 00:06:20.74 +54:44:20.6
116.39501 -7.55937 galactic Cas Second-epoch detections are separated by 0.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.5720+54.7461 | 00:06:20.66 +54:44:48.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:20.74 +54:44:20.6: 13.63 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:20.74 +54:44:20.6: 13.14 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 06 20.74 +54 44 20.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.5720+54.7461,2461238.6600,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.5720+54.7461 20260717.1600 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.11 23:58:38.58 +53:54:04.6
115.12095 -8.16787 galactic Cas Second-epoch detections are separated by 0.7" and 1.2 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 J359.6649+53.9052 | 23:58:38.58 +53:54:04.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.368+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:38.58 +53:54:04.6: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:38.58 +53:54:04.6: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 58 38.58 +53 54 04.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.6649+53.9052,2461238.6600,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.6649+53.9052 20260717.1600 11.11CV 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 17.1600 2461238.6600 10.87 00:30:31.18 +55:56:24.5
119.98503 -6.81187 galactic Cas Second-epoch detections are separated by 1.7" and 1.5 pix
The object was found in VSX22" Gaia DR3 421275548023447040
Type: VAR
# Max. Min./Amp. JD0 Period
14.690 G 14.700 G 0.023349900000 K
ATTENTION: measured mag 10.87 is 3.8 mag brighter than the VSX record maximum brightness 14.69 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:31.18 +55:56:24.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:31.18 +55:56:24.5: 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 17.1600* 00 30 31.18 +55 56 24.5 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421275548023447040,2461238.6600,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421275548023447040 20260717.1600 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.11 23:13:06.15 +53:45:12.2
108.60213 -6.35998 galactic Cas Second-epoch detections are separated by 0.6" and 1.0 pix
The object was found in VSX23" ZTF J231308.58+534520.0
Type: M
# Max. Min./Amp. JD0 Period
19.454 g Y 4.908 g 2458360.34240 358.008827700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:06.15 +53:45:12.2: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:06.15 +53:45:12.2: 13.30 +/- 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 17.1600* 23 13 06.15 +53 45 12.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J231308.58+534520.0,2461238.6600,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J231308.58+534520.0 20260717.1600 11.11CV 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 17.1600 2461238.6600 10.65 00:19:09.98 +52:36:33.5
117.96810 -9.95113 galactic Cas Second-epoch detections are separated by 0.5" and 1.4 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 419146098938074112 | 00:19:09.81 +52:36:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.286+/-0.031 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:09.98 +52:36:33.5: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:09.98 +52:36:33.5: 13.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 19 09.98 +52 36 33.5 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
Gaia DR3 419146098938074112,2461238.6600,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419146098938074112 20260717.1600 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.02 23:18:56.70 +53:20:37.3
109.26704 -7.05628 galactic Cas Second-epoch detections are separated by 0.5" and 1.0 pix
The object was found in VSX 2" Gaia DR3 1995687275993223168
Type: ROT
# Max. Min./Amp. JD0 Period
12.980 G 13.010 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.70 +53:20:37.3: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:56.70 +53:20:37.3: 13.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 18 56.70 +53 20 37.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995687275993223168,2461238.6600,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995687275993223168 20260717.1600 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.15 23:12:41.18 +54:49:13.0
108.94546 -5.34741 galactic Cas Second-epoch detections are separated by 1.3" and 1.1 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 1996494626770732160 | 23:12:37.83 +54:49:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:41.18 +54:49:13.0: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:41.18 +54:49:13.0: 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 17.1600* 23 12 41.18 +54 49 13.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996494626770732160,2461238.6600,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996494626770732160 20260717.1600 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.03 23:10:02.58 +56:51:40.1
109.37349 -3.31750 galactic Cas Second-epoch detections are separated by 1.9" and 0.9 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 J347.5055+56.8648 | 23:10:04.48 +56:52:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:02.58 +56:51:40.1: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:02.58 +56:51:40.1: 13.35 +/- 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 17.1600* 23 10 02.58 +56 51 40.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.5055+56.8648,2461238.6600,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.5055+56.8648 20260717.1600 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 10.73 23:46:36.45 +51:42:14.5
112.81916 -9.89024 galactic Cas Second-epoch detections are separated by 0.6" and 1.3 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 1945016110828646912 | 23:46:35.08 +51:42:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.706+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:36.45 +51:42:14.5: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:36.45 +51:42:14.5: 13.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 46 36.45 +51 42 14.5 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
Gaia DR3 1945016110828646912,2461238.6600,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1945016110828646912 20260717.1600 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 17.1600 2461238.6600 10.55 00:13:40.71 +56:53:48.4
117.76808 -5.59591 galactic Cas Second-epoch detections are separated by 0.4" and 1.2 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 J003.4030+56.9099 | 00:13:37.40 +56:53:50.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.766+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:40.71 +56:53:48.4: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:40.71 +56:53:48.4: 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 17.1600* 00 13 40.71 +56 53 48.4 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 J003.4030+56.9099,2461238.6600,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.4030+56.9099 20260717.1600 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 17.1600 2461238.6600 10.96 23:20:46.33 +53:39:16.9
109.63287 -6.85960 galactic Cas Second-epoch detections are separated by 2.4" and 1.3 pix
The object was found in VSX20" ASASSN-V J232046.82+533857.7
Type: L
# Max. Min./Amp. JD0 Period
11.070 V 11.170 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:46.33 +53:39:16.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:46.33 +53:39:16.9: 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 17.1600* 23 20 46.33 +53 39 16.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J232046.82+533857.7,2461238.6600,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J232046.82+533857.7 20260717.1600 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 10.44 00:24:24.45 +57:11:31.3
119.25963 -5.48686 galactic Cas Second-epoch detections are separated by 0.9" and 1.3 pix
The object was found in VSX16" Gaia DR3 421969064983111296
Type: ROT
# Max. Min./Amp. JD0 Period
15.450 G 15.490 G F
ATTENTION: measured mag 10.44 is 5.0 mag brighter than the VSX record maximum brightness 15.45 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:24.45 +57:11:31.3: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:24.45 +57:11:31.3: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 24 24.45 +57 11 31.3 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421969064983111296,2461238.6600,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421969064983111296 20260717.1600 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 17.1600 2461238.6600 10.31 23:33:10.46 +52:52:20.6
111.14778 -8.19938 galactic Cas Second-epoch detections are separated by 1.1" and 1.1 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 1993221548150793472 | 23:33:14.36 +52:52:24.7 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.153+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:10.46 +52:52:20.6: 13.12 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:10.46 +52:52:20.6: 12.84 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 17.1600* 23 33 10.46 +52 52 20.6 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 1993221548150793472,2461238.6600,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993221548150793472 20260717.1600 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 9.62 00:15:19.54 +53:12:02.4
117.46651 -9.28744 galactic Cas Second-epoch detections are separated by 0.5" and 1.4 pix
The object was found in VSX 1" Gaia DR3 419244578251557888
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.410 G 11.480 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:19.54 +53:12:02.4: 13.29 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:19.54 +53:12:02.4: 13.22 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 17.1600* 00 15 19.54 +53 12 02.4 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 419244578251557888,2461238.6600,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419244578251557888 20260717.1600 9.62CV 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 17.1600 2461238.6600 9.20 23:15:52.58 +52:57:58.3
108.69798 -7.24421 galactic And Second-epoch detections are separated by 2.9" and 1.4 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 J348.9601+52.9506 | 23:15:51.87 +52:57:37.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1927AnHar.100...33C HD 236076 J-Ks=0.396+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:52.58 +52:57:58.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:52.58 +52:57:58.3: 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 17.1600* 23 15 52.58 +52 57 58.3 9.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.9601+52.9506,2461238.6600,9.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.9601+52.9506 20260717.1600 9.20CV 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 17.1600 2461238.6600 10.27 23:43:27.95 +50:54:08.4
112.12669 -10.53784 galactic Cas Second-epoch detections are separated by 0.8" and 1.4 pix
The object was found in VSX 6" Gaia DR3 1943854751672564096
Type: RS
# Max. Min./Amp. JD0 Period
15.050 G 15.130 G K
ATTENTION: measured mag 10.27 is 4.8 mag brighter than the VSX record maximum brightness 15.05 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:27.95 +50:54:08.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:27.95 +50:54:08.4: 13.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 43 27.95 +50 54 08.4 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 1943854751672564096,2461238.6600,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943854751672564096 20260717.1600 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 17.1600 2461238.6600 11.61 23:12:17.67 +57:05:09.0
109.74301 -3.22532 galactic Cas Second-epoch detections are separated by 1.4" and 0.7 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 J348.0943+57.0885 | 23:12:17.67 +57:05:09.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:17.67 +57:05:09.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:17.67 +57:05:09.0: 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 17.1600* 23 12 17.67 +57 05 09.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.0943+57.0885,2461238.6600,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.0943+57.0885 20260717.1600 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.57 23:25:27.95 +49:20:12.5
108.84746 -11.16947 galactic And Second-epoch detections are separated by 2.3" and 1.8 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 | 23:25:27.95 +49:20:12.5 (user input) | T | P | (position from user input) J-Ks=0.648+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:27.95 +49:20:12.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:27.95 +49:20:12.5: 13.51 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.51 +/- 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 17.1600* 23 25 27.95 +49 20 12.5 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.48 23:26:01.34 +49:55:47.2
109.13397 -10.63976 galactic And Second-epoch detections are separated by 1.2" and 1.1 pix
The object was found in VSX 4" Gaia DR3 1943087155117309568
Type:
# Max. Min./Amp. JD0 Period
14.000 G 14.030 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:01.34 +49:55:47.2: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:01.34 +49:55:47.2: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 26 01.34 +49 55 47.2 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943087155117309568,2461238.6600,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943087155117309568 20260717.1600 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.29 00:14:30.86 +56:43:29.5
117.85675 -5.78260 galactic Cas Second-epoch detections are separated by 0.4" and 1.2 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 J003.6271+56.7453 | 00:14:30.53 +56:44:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=1.189+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:30.86 +56:43:29.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:30.86 +56:43:29.5: 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 17.1600* 00 14 30.86 +56 43 29.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.6271+56.7453,2461238.6600,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.6271+56.7453 20260717.1600 11.29CV 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 17.1600 2461238.6600 11.45 23:33:41.01 +49:58:07.5
110.33698 -10.99194 galactic And Second-epoch detections are separated by 1.7" and 1.6 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 J353.4219+49.9732 | 23:33:43.36 +49:58:40.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 1952CoRut..32....1H BD+49 4154 J-Ks=0.388+/-0.031 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:41.01 +49:58:07.5: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:41.01 +49:58:07.5: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 33 41.01 +49 58 07.5 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.4219+49.9732,2461238.6600,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.4219+49.9732 20260717.1600 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.63 23:41:50.01 +54:40:26.7
112.90200 -6.83653 galactic Cas Second-epoch detections are separated by 1.6" and 1.3 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 J355.4769+54.6722 | 23:41:50.01 +54:40:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.736+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:50.01 +54:40:26.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:50.01 +54:40:26.7: 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 17.1600* 23 41 50.01 +54 40 26.7 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.4769+54.6722,2461238.6600,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.4769+54.6722 20260717.1600 11.63CV 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 17.1600 2461238.6600 11.68 23:34:08.29 +54:02:58.4
111.64100 -7.11894 galactic Cas Second-epoch detections are separated by 3.4" and 1.1 pix
The object was found in VSX 1" Gaia DR3 1994286807419596416
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.630 G 13.670 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.29 +54:02:58.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.29 +54:02:58.4: 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 17.1600* 23 34 08.29 +54 02 58.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994286807419596416,2461238.6600,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994286807419596416 20260717.1600 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.95 23:21:05.80 +55:55:39.5
110.46336 -4.74161 galactic Cas Second-epoch detections are separated by 2.3" and 0.9 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 | 23:21:05.80 +55:55:39.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:05.80 +55:55:39.5: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:05.80 +55:55:39.5: 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 17.1600* 23 21 05.80 +55 55 39.5 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.82 23:24:53.16 +54:29:06.1
110.48698 -6.28196 galactic Cas Second-epoch detections are separated by 0.6" and 0.9 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 | 23:24:53.16 +54:29:06.1 (user input) | T | P | (position from user input) J-Ks=0.790+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:53.16 +54:29:06.1: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:53.16 +54:29:06.1: 13.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 24 53.16 +54 29 06.1 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.78 23:11:51.35 +55:18:28.6
109.01823 -4.85072 galactic Cas Second-epoch detections are separated by 5.0" and 1.7 pix
The object was found in VSX 5" Gaia DR3 1996757100812082688
Type: ROT
# Max. Min./Amp. JD0 Period
13.540 G 13.560 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:51.35 +55:18:28.6: 13.62 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:51.35 +55:18:28.6: 13.23 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 11 51.35 +55 18 28.6 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996757100812082688,2461238.6600,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996757100812082688 20260717.1600 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.81 23:29:18.29 +50:38:17.6
109.87137 -10.13900 galactic And Second-epoch detections are separated by 3.9" and 1.8 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 1943250363874965504 | 23:29:16.73 +50:38:53.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:18.29 +50:38:17.6: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:18.29 +50:38:17.6: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 29 18.29 +50 38 17.6 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943250363874965504,2461238.6600,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943250363874965504 20260717.1600 11.81CV 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 17.1600 2461238.6600 11.89 23:28:27.72 +53:49:29.8
110.77040 -7.07602 galactic Cas Second-epoch detections are separated by 5.7" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.1131+53.8121 | 23:28:30.29 +53:48:52.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:27.72 +53:49:29.8: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:27.72 +53:49:29.8: 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 17.1600* 23 28 27.72 +53 49 29.8 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.1131+53.8121,2461238.6600,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.1131+53.8121 20260717.1600 11.89CV 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 17.1600 2461238.6600 11.72 23:58:30.70 +56:50:31.0
115.70932 -5.28577 galactic Cas Second-epoch detections are separated by 0.4" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J359.6079+56.8364 | 23:58:27.91 +56:50:04.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.049+/-0.036 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:30.70 +56:50:31.0: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:30.70 +56:50:31.0: 13.26 +/- 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 17.1600* 23 58 30.70 +56 50 31.0 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.6079+56.8364,2461238.6600,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.6079+56.8364 20260717.1600 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.72 00:11:12.46 +57:36:24.6
117.54430 -4.84347 galactic Cas Second-epoch detections are separated by 2.1" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J002.8033+57.5971 | 00:11:12.46 +57:36:24.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.282+/-0.046 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:12.46 +57:36:24.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:12.46 +57:36:24.6: 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 17.1600* 00 11 12.46 +57 36 24.6 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.8033+57.5971,2461238.6600,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J002.8033+57.5971 20260717.1600 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.71 23:49:51.83 +52:07:56.1
113.41982 -9.59864 galactic Cas Second-epoch detections are separated by 2.3" and 1.7 pix
The object was found in VSX 4" ASASSN-V J234951.66+520759.8
Type: SR
# Max. Min./Amp. JD0 Period
13.740 V 14.440 V 2458507.39130 134.115277600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:51.83 +52:07:56.1: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:51.83 +52:07:56.1: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 49 51.83 +52 07 56.1 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J234951.66+520759.8,2461238.6600,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J234951.66+520759.8 20260717.1600 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 11.72 00:04:53.61 +51:59:42.5
115.68234 -10.22024 galactic Cas Second-epoch detections are separated by 3.0" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.2174+52.0011 | 00:04:53.61 +51:59:42.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:53.61 +51:59:42.5: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:53.61 +51:59:42.5: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 04 53.61 +51 59 42.5 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.2174+52.0011,2461238.6600,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.2174+52.0011 20260717.1600 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.07 23:28:08.32 +53:01:02.4
110.46492 -7.82622 galactic Cas Second-epoch detections are separated by 0.8" and 1.2 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 1992531608904014080 | 23:28:10.38 +53:01:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.371+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:08.32 +53:01:02.4: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:08.32 +53:01:02.4: 13.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 28 08.32 +53 01 02.4 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992531608904014080,2461238.6600,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992531608904014080 20260717.1600 12.07CV 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 17.1600 2461238.6600 12.18 23:16:57.02 +54:01:33.6
109.23333 -6.31357 galactic Cas Second-epoch detections are separated by 4.9" and 1.8 pix
The object was found in VSX17" ZTF J231656.43+540117.9
Type: BY
# Max. Min./Amp. JD0 Period
16.668 r Y 0.065 r 2458386.77740 0.683370600000
ATTENTION: measured mag 12.18 is 4.4 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-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:57.02 +54:01:33.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:57.02 +54:01:33.6: 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 17.1600* 23 16 57.02 +54 01 33.6 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J231656.43+540117.9,2461238.6600,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J231656.43+540117.9 20260717.1600 12.18CV 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 17.1600 2461238.6600 12.05 23:32:21.35 +53:10:39.0
111.12252 -7.87133 galactic Cas Second-epoch detections are separated by 0.3" and 1.2 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 J353.0827+53.1779 | 23:32:21.35 +53:10:39.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.855+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:21.35 +53:10:39.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:21.35 +53:10:39.0: 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 17.1600* 23 32 21.35 +53 10 39.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.0827+53.1779,2461238.6600,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.0827+53.1779 20260717.1600 12.05CV 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 17.1600 2461238.6600 12.01 23:26:28.94 +53:45:56.0
110.47222 -7.03834 galactic Cas Second-epoch detections are separated by 2.1" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J351.6210+53.7677 | 23:26:28.94 +53:45:56.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:28.94 +53:45:56.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:28.94 +53:45:56.0: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 26 28.94 +53 45 56.0 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.6210+53.7677,2461238.6600,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.6210+53.7677 20260717.1600 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 17.1600 2461238.6600 12.31 23:14:46.41 +54:27:10.1
109.09085 -5.80051 galactic Cas Second-epoch detections are separated by 1.5" and 1.0 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 | 23:14:46.41 +54:27:10.1 (user input) | T | P | (position from user input) J-Ks=0.766+/-0.037 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:46.41 +54:27:10.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:46.41 +54:27:10.1: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 14 46.41 +54 27 10.1 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461238.6600,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.1600 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.01 00:10:04.53 +50:47:22.2
116.28107 -11.54734 galactic Cas Second-epoch detections are separated by 6.5" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J002.5137+50.7986 | 00:10:04.53 +50:47:22.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.826+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:04.53 +50:47:22.2: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:04.53 +50:47:22.2: 13.28 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 17.1600* 00 10 04.53 +50 47 22.2 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.5137+50.7986,2461238.6600,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J002.5137+50.7986 20260717.1600 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 17.1600 2461238.6600 12.49 23:31:29.93 +54:52:04.1
111.52108 -6.22315 galactic Cas Second-epoch detections are separated by 2.5" and 1.2 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 1997372445060778368 | 23:31:27.22 +54:52:35.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.411+/-0.041 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:29.93 +54:52:04.1: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:29.93 +54:52:04.1: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 31 29.93 +54 52 04.1 12.5 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 1997372445060778368,2461238.6600,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997372445060778368 20260717.1600 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.28 00:03:26.43 +54:10:35.2
115.87304 -8.03616 galactic Cas Second-epoch detections are separated by 2.1" and 1.6 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 420321584247717120 | 00:03:27.84 +54:11:04.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.322+/-0.073 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:26.43 +54:10:35.2: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:26.43 +54:10:35.2: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 00 03 26.43 +54 10 35.2 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420321584247717120,2461238.6600,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420321584247717120 20260717.1600 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.60 23:49:03.98 +55:05:29.8
114.02195 -6.69750 galactic Cas Second-epoch detections are separated by 2.7" and 1.3 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 1994589757232914560 | 23:49:00.14 +55:05:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.431+/-0.038 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:03.98 +55:05:29.8: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:03.98 +55:05:29.8: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.1600* 23 49 03.98 +55 05 29.8 12.6 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 1994589757232914560,2461238.6600,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994589757232914560 20260717.1600 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 12.52 00:03:48.68 +56:35:45.5
116.37765 -5.66848 galactic Cas Second-epoch detections are separated by 2.5" and 1.0 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 421027298907188736 | 00:03:45.30 +56:35:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.671+/-0.036 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:48.68 +56:35:45.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:48.68 +56:35:45.5: 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 17.1600* 00 03 48.68 +56 35 45.5 12.5 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 421027298907188736,2461238.6600,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421027298907188736 20260717.1600 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.1600 2461238.6600 10.87 23:21:12.04 +50:00:12.4
108.41734 -10.30806 galactic And Second-epoch detections are separated by 0.4" and 1.4 pix
The object was found in VSX 4" AK And
Type: M
# Max. Min./Amp. JD0 Period
10.000 V < 15.000 V 2452930.00000 317.000000000000 S:
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:12.04 +50:00:12.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:12.04 +50:00:12.4: 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 17.1600* 23 21 12.04 +50 00 12.4 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AK And,2461238.6600,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AK And 20260717.1600 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461238.66022464 17.07.2026 03:50:33.409 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 18 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): 21638
Objects passed selection criteria: 21591
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 18468
Average stars matched: 17520 (94.8668 %)
Memory usage VmPeak: 131332 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 16 05:04:38 CDT 2026
VaST build number 1.0rc89-156-g3b0d8dc3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 22:58:46 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461238.66022464 17.07.2026 03:50:33.409 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 334
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 291 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): 163484
Objects passed selection criteria: 163124
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 146771
Average stars matched: 139899 (95.3179 %)
Memory usage VmPeak: 1939644 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 16 05:04:38 CDT 2026
VaST build number 1.0rc89-156-g3b0d8dc3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 23:08:40 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.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: 2461238.65976169
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:57.586 +54:01:07.73 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
Image size: 939.8'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.673 +53:59:47.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.673 +53:59:47.08
Angular distance between the image centers 0.0256 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
Image size: 939.8'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.075 +53:59:41.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.075 +53:59:41.59
Angular distance between the image centers 0.0263 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:02.673 +53:59:47.08
Second-epoch second image center 00:00:02.075 +53:59:41.59
Angular distance between the image centers 0.00211 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.q8KBs9HLKP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.hJW880Vdcm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits &> /tmp/tmp.iflBjZYKzM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits &> /tmp/tmp.DRswdlmilE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9998 deg, Dec +48.2682 to +59.2677 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 0.0012 to 359.9998 deg, Dec 48.2682 to 59.2677 deg
Loaded 153348 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
ERROR: only 52 of 28951 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.18%) - 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 22.575300
a=0.000000 b=1.000000 c=22.575300
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.91
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.91
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9998 deg, Dec +48.2682 to +59.2677 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 0.0012 to 359.9998 deg, Dec 48.2682 to 59.2677 deg
Loaded 153348 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=6.3)
Read 32399 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0011 to 359.9996 deg, Dec +48.2682 to +59.2618 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 0.0011 to 359.9996 deg, Dec 48.2682 to 59.2618 deg
Loaded 153285 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): 56 out of 62 total matches.
Matched with Tycho-2 62 out of 32399 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.3 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
2.4 pix wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.3 pix wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Limiting magnitude estimates:
14.9 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
15.0 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (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.q8KBs9HLKP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2748, bad_region=6855, passed=28951
Got 28951 stars (including 19826 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 28951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (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 345.0821 through 0 to 14.9840, gap 14.9840 to 345.0821
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 241 matched stars entering correct_measured_positions(), 177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.18"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 235 matched stars entering correct_measured_positions(), 5819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.02"
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 345.0724 through 0 to 15.0101, gap 15.0101 to 345.0724
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 401 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 345 matched stars entering correct_measured_positions(), 5883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.97"
Accuracy estimation diagnostic: 341 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.85"
Excluding outliers - 341 stars left (next iteration limit 258)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=341 sigma_overall_arcsec=10.000 sigma_q1_arcsec=26.458 sigma_q2_arcsec=26.280 sigma_q3_arcsec=7.321 sigma_q4_arcsec=8.000 n_q1=41 n_q2=24 n_q3=122 n_q4=154 worst_quadrant_to_overall_ratio=2.646
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hJW880Vdcm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3204, bad_region=7312, passed=32399
Got 32399 stars (including 22421 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 32399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0823 through 0 to 14.9840, gap 14.9840 to 345.0823
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 320 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 234 matched stars entering correct_measured_positions(), 171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 6406 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
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 345.0732 through 0 to 15.0096, gap 15.0096 to 345.0732
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 399 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 343 matched stars entering correct_measured_positions(), 6467 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.48"
Accuracy estimation diagnostic: 340 matched stars entering correct_measured_positions(), 9572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.44"
Excluding outliers - 340 stars left (next iteration limit 248)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=340 sigma_overall_arcsec=11.206 sigma_q1_arcsec=29.679 sigma_q2_arcsec=28.591 sigma_q3_arcsec=8.393 sigma_q4_arcsec=9.911 n_q1=41 n_q2=25 n_q3=115 n_q4=159 worst_quadrant_to_overall_ratio=2.649
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.iflBjZYKzM (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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1246, bad_region=3027, passed=16560
Got 16560 stars (including 12462 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat
util/solve_plate_with_UCAC5 got 16560 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.8'
Seting catalog search parameters based on the expected field of view 939.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013053 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010442 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8475 through 0 to 14.6558, gap 14.6558 to 344.8475
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 13914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8480 through 0 to 14.6561, gap 14.6561 to 344.8480
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 13913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 13913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits N_match=974 sigma_overall_arcsec=0.629 sigma_q1_arcsec=0.644 sigma_q2_arcsec=0.605 sigma_q3_arcsec=0.690 sigma_q4_arcsec=0.565 n_q1=316 n_q2=175 n_q3=291 n_q4=192 worst_quadrant_to_overall_ratio=1.098
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.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.DRswdlmilE (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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1222, bad_region=3015, passed=16619
Got 16619 stars (including 12548 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat
util/solve_plate_with_UCAC5 got 16619 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.8'
Seting catalog search parameters based on the expected field of view 939.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013053 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010442 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8479 through 0 to 14.6559, gap 14.6559 to 344.8479
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8478 through 0 to 14.6562, gap 14.6562 to 344.8478
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits N_match=973 sigma_overall_arcsec=0.624 sigma_q1_arcsec=0.679 sigma_q2_arcsec=0.630 sigma_q3_arcsec=0.631 sigma_q4_arcsec=0.589 n_q1=321 n_q2=171 n_q3=297 n_q4=184 worst_quadrant_to_overall_ratio=1.087
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits sigma_overall=10.000 worst_q_ratio=2.646
ref2=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits sigma_overall=11.206 worst_q_ratio=2.649
new1=fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits sigma_overall=0.629 worst_q_ratio=1.098
new2=fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits sigma_overall=0.624 worst_q_ratio=1.087
reference average sigma_overall=10.603 worst_q_ratio=2.6475
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468_astrometric_residuals.png (341 matched stars from wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.98 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450_astrometric_residuals.png (340 matched stars from wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.94 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062_astrometric_residuals.png (974 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.57 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063_astrometric_residuals.png (973 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:12.27 +57:51:06.2: 15.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:29.93 +52:53:05.9: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:12.27 +57:51:06.2: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:29.93 +52:53:05.9: 15.64 +/- 99.00 upperlimit
Adding exclusion_list_gaiadr2.txt__out33555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33760.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33555_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 33555_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:37:29.93 +52:53:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.272 1993176266314810880 354.37412315553 +52.88496213032 11.9094 11.2128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33760_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 33760_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:28:12.27 +57:51:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 2.845 2010881908215321472 352.05027736062 +57.85237109963 12.0526 11.5202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21482_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 21482_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:44:31.92 +56:34:50.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07077_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 07077_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:09:36.47 +51:34:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06239_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 06239_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:58:25.15 +51:23:24.1 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 926.8'x616.3' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 23:59:57.586 +54:01:07.73 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
Image size: 939.8'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.673 +53:59:47.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.673 +53:59:47.08
Angular distance between the image centers 0.0256 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
Image size: 939.8'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:02.075 +53:59:41.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.075 +53:59:41.59
Angular distance between the image centers 0.0263 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:02.673 +53:59:47.08
Second-epoch second image center 00:00:02.075 +53:59:41.59
Angular distance between the image centers 0.00211 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.WwIe5mY15B
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.WBwHgT9S9P
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits &> /tmp/tmp.bb2YYgv1or
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits &> /tmp/tmp.kbQFaGQXqU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9998 deg, Dec +48.2503 to +59.2677 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 0.0002 to 359.9998 deg, Dec 48.2503 to 59.2677 deg
Loaded 153589 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): 104 out of 148 total matches.
Matched with Tycho-2 148 out of 200953 detected stars.
ERROR: only 104 of 200953 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.05%) - 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 20.521000
a=0.000000 b=1.000000 c=20.521000
From vast_summary.log: estimated ref. image limiting mag.: -7.31
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 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9998 deg, Dec +48.2503 to +59.2677 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 0.0002 to 359.9998 deg, Dec 48.2503 to 59.2677 deg
Loaded 153589 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): 104 out of 148 total matches.
Matched with Tycho-2 148 out of 200953 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=4.7)
Read 213202 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9999 deg, Dec +48.2308 to +59.2649 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 0.0002 to 359.9999 deg, Dec 48.2308 to 59.2649 deg
Loaded 153847 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): 122 out of 166 total matches.
Matched with Tycho-2 166 out of 213202 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 243 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.2 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Limiting magnitude estimates:
13.2 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
13.3 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
12.6 mag. fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
12.6 mag. fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.0 (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.WwIe5mY15B (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=60, blended=29230, bad_region=30798, passed=200893
Got 200893 stars (including 144443 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 200893 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (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 345.0121 through 0 to 15.0290, gap 15.0290 to 345.0121
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 326 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 236 matched stars entering correct_measured_positions(), 169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 225 matched stars entering correct_measured_positions(), 42039 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.34"
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 345.0161 through 0 to 15.0639, gap 15.0639 to 345.0161
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 402 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 42110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.32"
Accuracy estimation diagnostic: 341 matched stars entering correct_measured_positions(), 65834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.71"
Excluding outliers - 341 stars left (next iteration limit 247)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=341 sigma_overall_arcsec=10.173 sigma_q1_arcsec=28.653 sigma_q2_arcsec=29.926 sigma_q3_arcsec=7.272 sigma_q4_arcsec=10.943 n_q1=31 n_q2=26 n_q3=117 n_q4=167 worst_quadrant_to_overall_ratio=2.942
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WBwHgT9S9P (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=33709, bad_region=29431, passed=213150
Got 213150 stars (including 154424 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 213150 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0123 through 0 to 15.0317, gap 15.0317 to 345.0123
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 319 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 236 matched stars entering correct_measured_positions(), 166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 227 matched stars entering correct_measured_positions(), 46390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0158 through 0 to 15.0663, gap 15.0663 to 345.0158
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 395 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 46448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.44"
Accuracy estimation diagnostic: 332 matched stars entering correct_measured_positions(), 66751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.69"
Excluding outliers - 332 stars left (next iteration limit 249)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=332 sigma_overall_arcsec=11.113 sigma_q1_arcsec=28.693 sigma_q2_arcsec=26.729 sigma_q3_arcsec=8.129 sigma_q4_arcsec=9.837 n_q1=36 n_q2=26 n_q3=118 n_q4=152 worst_quadrant_to_overall_ratio=2.582
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bb2YYgv1or (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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=13558, bad_region=18001, passed=136543
Got 136543 stars (including 106138 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat
util/solve_plate_with_UCAC5 got 136543 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.8'
Seting catalog search parameters based on the expected field of view 939.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013053 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010442 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8096 through 0 to 14.7936, gap 14.7936 to 344.8096
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 121173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8094 through 0 to 14.7940, gap 14.7940 to 344.8094
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 121174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 121174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits N_match=977 sigma_overall_arcsec=0.619 sigma_q1_arcsec=0.633 sigma_q2_arcsec=0.598 sigma_q3_arcsec=0.682 sigma_q4_arcsec=0.599 n_q1=319 n_q2=182 n_q3=275 n_q4=201 worst_quadrant_to_overall_ratio=1.101
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.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.kbQFaGQXqU (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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=13033, bad_region=17898, passed=135502
Got 135502 stars (including 105680 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat
util/solve_plate_with_UCAC5 got 135502 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.8'
Seting catalog search parameters based on the expected field of view 939.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013053 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010442 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8079 through 0 to 14.7949, gap 14.7949 to 344.8079
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 120378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8076 through 0 to 14.7952, gap 14.7952 to 344.8076
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 120377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 120377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits N_match=975 sigma_overall_arcsec=0.649 sigma_q1_arcsec=0.650 sigma_q2_arcsec=0.634 sigma_q3_arcsec=0.675 sigma_q4_arcsec=0.640 n_q1=315 n_q2=185 n_q3=275 n_q4=200 worst_quadrant_to_overall_ratio=1.041
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-49-53_20.00sec_5.00C_LIGHT_0062.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.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_2026-07-16_CI_Cas-04-Q2b1x1_225426_TTUQ2b1x1_3245260_D4xuxg4m/wcs_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:00.60 +53:39:35.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:11.10 +55:35:59.3: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:34.69 +55:29:44.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:22.19 +53:38:21.0: 11.75 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:33.06 +53:02:41.7: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:47.52 +56:08:36.5: 13.49 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:10.44 +57:04:44.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:13.02 +56:04:31.5: 12.43 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:24.01 +54:46:43.2: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:11.10 +55:35:59.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:34.69 +55:29:44.7: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:00.60 +53:39:35.5: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:22.19 +53:38:21.0: 11.41 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:47.52 +56:08:36.5: 13.06 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:24.01 +54:46:43.2: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:33.06 +53:02:41.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:53:13.02 +56:04:31.5: 12.05 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:10.44 +57:04:44.9: 13.51 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.20 +/- 0.08
Forced photometry reference-image weighted average: 13.22 +/- 0.16
Forced photometry filter REJECTED candidate at 23:53:13.02 +56:04:31.5: ref_mag=12.20 +/- 0.08 new_mean_mag=12.4888 delta=-0.29 (need > 0.90)
Forced photometry reference-image weighted average: 11.56 +/- 0.04
Forced photometry filter KEPT candidate at 00:01:47.52 +56:08:36.5: ref_mag=13.22 +/- 0.16 new_mean_mag=12.0464 delta=1.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:15:22.19 +53:38:21.0: ref_mag=11.56 +/- 0.04 new_mean_mag=12.4777 delta=-0.92 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:43.11 +51:35:38.7: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:43.11 +51:35:38.7: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:05:06.39 +54:18:27.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:01.45 +53:17:43.1: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:05:06.39 +54:18:27.5: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:01.45 +53:17:43.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:22.42 +54:06:37.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:22.42 +54:06:37.2: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:18.41 +55:48:26.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:18.41 +55:48:26.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:39.42 +53:29:42.5: 10.99 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:07.72 +56:06:31.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:39.42 +53:29:42.5: 10.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.02
Forced photometry filter REJECTED candidate at 00:03:39.42 +53:29:42.5: ref_mag=10.83 +/- 0.02 new_mean_mag=11.9742 delta=-1.14 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:01.72 +55:52:34.1: 10.81 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:07.72 +56:06:31.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:43.25 +57:15:39.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:01.72 +55:52:34.1: 10.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.69 +/- 0.01
Forced photometry filter REJECTED candidate at 23:56:01.72 +55:52:34.1: ref_mag=10.69 +/- 0.01 new_mean_mag=11.9203 delta=-1.23 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:47.75 +57:16:15.6: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:43.25 +57:15:39.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:40:06.44 +54:53:06.6: 12.91 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:47.75 +57:16:15.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:18.26 +52:16:23.0: 13.25 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:34.69 +54:09:02.7: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:40:06.44 +54:53:06.6: 12.75 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.12
Forced photometry filter KEPT candidate at 23:40:06.44 +54:53:06.6: ref_mag=12.83 +/- 0.12 new_mean_mag=11.8783 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:34.69 +54:09:02.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:18.26 +52:16:23.0: 13.23 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:48.94 +51:38:41.5: 13.85 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.24 +/- 0.19
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:11.69 +57:06:26.0: 13.67 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 23:39:18.26 +52:16:23.0: ref_mag=13.24 +/- 0.19 new_mean_mag=12.0113 delta=1.23 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:48.94 +51:38:41.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:11.69 +57:06:26.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:31.28 +56:42:26.6: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:31.28 +56:42:26.6: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:51.26 +49:17:44.6: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:51.26 +49:17:44.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:17:02.06 +57:24:19.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:17:02.06 +57:24:19.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:18.03 +53:07:47.9: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:18.03 +53:07:47.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:03.35 +50:48:21.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:38:29.16 +57:59:55.6: 10.67 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:03.35 +50:48:21.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:38:29.16 +57:59:55.6: 10.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.44 +/- 0.01
Forced photometry filter REJECTED candidate at 23:38:29.16 +57:59:55.6: ref_mag=10.44 +/- 0.01 new_mean_mag=11.9943 delta=-1.56 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:10.53 +53:55:05.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:58.00 +56:09:30.6: 11.82 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:10.53 +53:55:05.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:58.00 +56:09:30.6: 11.57 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.04
Forced photometry filter REJECTED candidate at 23:52:58.00 +56:09:30.6: ref_mag=11.68 +/- 0.04 new_mean_mag=11.8737 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:37.95 +53:44:18.0: 12.74 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:37.95 +53:44:18.0: 12.45 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.10
Forced photometry filter REJECTED candidate at 00:00:37.95 +53:44:18.0: ref_mag=12.58 +/- 0.10 new_mean_mag=11.7329 delta=0.85 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:09.34 +52:19:40.5: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:00.11 +57:25:00.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:38.90 +53:36:25.0: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:09.34 +52:19:40.5: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:04.21 +54:39:05.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:00.11 +57:25:00.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:38.90 +53:36:25.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:18.96 +54:52:41.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:04.21 +54:39:05.3: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:18.96 +54:52:41.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:38:57.63 +54:45:08.9: 13.12 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:38:57.63 +54:45:08.9: 13.55 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.17
Forced photometry filter KEPT candidate at 23:38:57.63 +54:45:08.9: ref_mag=13.24 +/- 0.17 new_mean_mag=11.8122 delta=1.43 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:13.24 +56:39:04.0: 11.34 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:13.24 +56:39:04.0: 11.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.05
Forced photometry filter REJECTED candidate at 23:57:13.24 +56:39:04.0: ref_mag=11.19 +/- 0.05 new_mean_mag=11.7997 delta=-0.61 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:25.66 +51:54:37.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:25.66 +51:54:37.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:31.70 +55:18:15.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:05.99 +56:05:26.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:31.70 +55:18:15.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:55.82 +54:03:11.7: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:05.99 +56:05:26.7: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:55.82 +54:03:11.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:21.43 +51:55:17.7: 12.62 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:21.43 +51:55:17.7: 12.39 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.08
Forced photometry filter REJECTED candidate at 23:52:21.43 +51:55:17.7: ref_mag=12.50 +/- 0.08 new_mean_mag=11.6836 delta=0.81 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:59.36 +55:56:51.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:59.36 +55:56:51.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:28.24 +51:50:29.5: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:28.24 +51:50:29.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:52.96 +56:36:03.3: 12.49 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:57.54 +51:01:11.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:52.96 +56:36:03.3: 12.18 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.08
Forced photometry filter REJECTED candidate at 00:04:52.96 +56:36:03.3: ref_mag=12.32 +/- 0.08 new_mean_mag=11.5141 delta=0.80 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:57.54 +51:01:11.3: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:56.84 +57:43:36.4: 10.68 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:56.84 +57:43:36.4: 10.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.50 +/- 0.02
Forced photometry filter REJECTED candidate at 00:31:56.84 +57:43:36.4: ref_mag=10.50 +/- 0.02 new_mean_mag=11.2692 delta=-0.77 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:40.70 +56:24:47.6: 11.92 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:40.70 +56:24:47.6: 11.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.05
Forced photometry filter REJECTED candidate at 23:56:40.70 +56:24:47.6: ref_mag=11.79 +/- 0.05 new_mean_mag=11.3235 delta=0.46 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:28.17 +52:04:54.8: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:28.17 +52:04:54.8: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:17.84 +54:52:52.7: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:01.73 +55:14:39.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:17.84 +54:52:52.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:01.73 +55:14:39.2: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:56.67 +52:27:19.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:56.67 +52:27:19.8: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:53.64 +56:49:23.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:53.64 +56:49:23.2: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:28.15 +56:13:39.0: 10.56 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:18.47 +56:19:03.0: 13.22 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:43.76 +53:43:48.8: 12.04 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:18.47 +56:19:03.0: 13.11 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.17
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:28.15 +56:13:39.0: 10.27 +/- 0.02 detection
Forced photometry filter KEPT candidate at 23:18:18.47 +56:19:03.0: ref_mag=13.17 +/- 0.17 new_mean_mag=11.6146 delta=1.55 (need > 0.90)
Forced photometry reference-image weighted average: 10.40 +/- 0.01
Forced photometry filter REJECTED candidate at 23:56:28.15 +56:13:39.0: ref_mag=10.40 +/- 0.01 new_mean_mag=11.2869 delta=-0.88 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:43.76 +53:43:48.8: 11.80 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.06
Forced photometry filter REJECTED candidate at 00:11:43.76 +53:43:48.8: ref_mag=11.91 +/- 0.06 new_mean_mag=11.1278 delta=0.78 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:20.74 +54:44:20.6: 13.63 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:38.58 +53:54:04.6: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:20.74 +54:44:20.6: 13.14 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.19
Forced photometry filter KEPT candidate at 00:06:20.74 +54:44:20.6: ref_mag=13.30 +/- 0.19 new_mean_mag=11.0925 delta=2.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:21.86 +55:46:41.7: 8.56 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:21.86 +55:46:41.7: 8.25 +/- 0.00 detection
Forced photometry reference-image weighted average: 8.37 +/- 0.00
Forced photometry filter REJECTED candidate at 00:26:21.86 +55:46:41.7: ref_mag=8.37 +/- 0.00 new_mean_mag=10.9797 delta=-2.61 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:38.58 +53:54:04.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:31.18 +55:56:24.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:31.18 +55:56:24.5: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:06.15 +53:45:12.2: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:06.15 +53:45:12.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:09.98 +52:36:33.5: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:09.98 +52:36:33.5: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.70 +53:20:37.3: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:41.18 +54:49:13.0: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:02.58 +56:51:40.1: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:56.70 +53:20:37.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:41.18 +54:49:13.0: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:02.58 +56:51:40.1: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:36.45 +51:42:14.5: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:36.45 +51:42:14.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:40.71 +56:53:48.4: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:40.71 +56:53:48.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:46.33 +53:39:16.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:28.93 +54:56:19.2: 8.91 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:46.33 +53:39:16.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:28.93 +54:56:19.2: 8.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 8.76 +/- 0.00
Forced photometry filter REJECTED candidate at 23:52:28.93 +54:56:19.2: ref_mag=8.76 +/- 0.00 new_mean_mag=10.4587 delta=-1.70 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:24.45 +57:11:31.3: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:24.45 +57:11:31.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:10.46 +52:52:20.6: 13.12 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:19.54 +53:12:02.4: 13.29 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:10.46 +52:52:20.6: 12.84 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.14
Forced photometry filter KEPT candidate at 23:33:10.46 +52:52:20.6: ref_mag=12.97 +/- 0.14 new_mean_mag=10.3169 delta=2.65 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:19.54 +53:12:02.4: 13.22 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.17
Forced photometry filter KEPT candidate at 00:15:19.54 +53:12:02.4: ref_mag=13.26 +/- 0.17 new_mean_mag=9.6216 delta=3.64 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:52.58 +52:57:58.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:52.58 +52:57:58.3: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:27.95 +50:54:08.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:27.95 +50:54:08.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:55.35 +56:28:28.6: 10.80 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:55.35 +56:28:28.6: 10.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.64 +/- 0.03
Forced photometry filter REJECTED candidate at 23:57:55.35 +56:28:28.6: ref_mag=10.64 +/- 0.03 new_mean_mag=10.9082 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:56.56 +53:10:41.2: 9.71 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:56.56 +53:10:41.2: 9.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.46 +/- 0.01
Forced photometry filter REJECTED candidate at 23:17:56.56 +53:10:41.2: ref_mag=9.46 +/- 0.01 new_mean_mag=11.3689 delta=-1.91 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:48:29.76 +51:25:23.3: 12.06 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:17.67 +57:05:09.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:48:29.76 +51:25:23.3: 11.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.05
Forced photometry filter REJECTED candidate at 23:48:29.76 +51:25:23.3: ref_mag=11.98 +/- 0.05 new_mean_mag=11.2967 delta=0.68 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:17.67 +57:05:09.0: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:27.95 +49:20:12.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:27.95 +49:20:12.5: 13.51 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.34
Forced photometry filter KEPT candidate at 23:25:27.95 +49:20:12.5: ref_mag=13.51 +/- 0.34 new_mean_mag=11.5601 delta=1.94 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:01.34 +49:55:47.2: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:30.86 +56:43:29.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:01.34 +49:55:47.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:41.01 +49:58:07.5: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:30.86 +56:43:29.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:41.01 +49:58:07.5: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:50.01 +54:40:26.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.29 +54:02:58.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.29 +54:02:58.4: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:05.80 +55:55:39.5: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:50.01 +54:40:26.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:05.80 +55:55:39.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:53.16 +54:29:06.1: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:53.16 +54:29:06.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:13.43 +57:25:54.8: 9.48 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:13.43 +57:25:54.8: 9.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.30 +/- 0.00
Forced photometry filter REJECTED candidate at 00:00:13.43 +57:25:54.8: ref_mag=9.30 +/- 0.00 new_mean_mag=11.7093 delta=-2.41 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:51.35 +55:18:28.6: 13.62 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:51.35 +55:18:28.6: 13.23 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.22
Forced photometry filter KEPT candidate at 23:11:51.35 +55:18:28.6: ref_mag=13.38 +/- 0.22 new_mean_mag=11.7466 delta=1.63 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:18.29 +50:38:17.6: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:27.72 +53:49:29.8: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:18.29 +50:38:17.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:27.72 +53:49:29.8: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:30.70 +56:50:31.0: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:30.70 +56:50:31.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:12.46 +57:36:24.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:51.83 +52:07:56.1: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:12.46 +57:36:24.6: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:12.88 +54:21:38.7: 12.03 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:51.83 +52:07:56.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:12.88 +54:21:38.7: 11.86 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.06
Forced photometry filter REJECTED candidate at 23:52:12.88 +54:21:38.7: ref_mag=11.94 +/- 0.06 new_mean_mag=11.7282 delta=0.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:53.61 +51:59:42.5: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:53.61 +51:59:42.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:08:18.45 +54:03:28.3: 11.13 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:18.45 +54:03:28.3: 10.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.02
Forced photometry filter REJECTED candidate at 00:08:18.45 +54:03:28.3: ref_mag=10.96 +/- 0.02 new_mean_mag=11.7843 delta=-0.83 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:08.32 +53:01:02.4: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:08.32 +53:01:02.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:57.02 +54:01:33.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:58.48 +57:32:03.1: 10.53 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:57.02 +54:01:33.6: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:58.48 +57:32:03.1: 10.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.39 +/- 0.02
Forced photometry filter REJECTED candidate at 00:11:58.48 +57:32:03.1: ref_mag=10.39 +/- 0.02 new_mean_mag=11.8674 delta=-1.48 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:21.35 +53:10:39.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:28.94 +53:45:56.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:21.35 +53:10:39.0: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:28.94 +53:45:56.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:54.30 +56:41:21.5: 12.75 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:54.30 +56:41:21.5: 12.55 +/- 0.27 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.19
Forced photometry filter REJECTED candidate at 23:57:54.30 +56:41:21.5: ref_mag=12.65 +/- 0.19 new_mean_mag=11.9718 delta=0.68 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:55.86 +55:54:16.4: 12.48 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:51:55.86 +55:54:16.4: 12.31 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.11
Forced photometry filter REJECTED candidate at 23:51:55.86 +55:54:16.4: ref_mag=12.40 +/- 0.11 new_mean_mag=12.1445 delta=0.26 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:46.41 +54:27:10.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:32.70 +56:54:12.6: 12.25 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:46.41 +54:27:10.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:32.70 +56:54:12.6: 12.10 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.07
Forced photometry filter REJECTED candidate at 00:13:32.70 +56:54:12.6: ref_mag=12.18 +/- 0.07 new_mean_mag=11.9535 delta=0.23 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:04.53 +50:47:22.2: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:04.53 +50:47:22.2: 13.28 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.25
Forced photometry filter KEPT candidate at 00:10:04.53 +50:47:22.2: ref_mag=13.28 +/- 0.25 new_mean_mag=11.9929 delta=1.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:13.09 +51:30:53.8: 11.24 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:13.09 +51:30:53.8: 10.77 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.94 +/- 0.02
Forced photometry filter REJECTED candidate at 23:20:13.09 +51:30:53.8: ref_mag=10.94 +/- 0.02 new_mean_mag=12.3654 delta=-1.42 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:29.93 +54:52:04.1: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:30.03 +55:43:32.3: 12.11 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:29.93 +54:52:04.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:30.03 +55:43:32.3: 11.97 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.06
Forced photometry filter REJECTED candidate at 23:50:30.03 +55:43:32.3: ref_mag=12.04 +/- 0.06 new_mean_mag=12.5186 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:45.28 +55:06:19.1: 12.10 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:45.28 +55:06:19.1: 11.68 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.05
Forced photometry filter REJECTED candidate at 23:31:45.28 +55:06:19.1: ref_mag=11.84 +/- 0.05 new_mean_mag=12.5937 delta=-0.76 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:26.43 +54:10:35.2: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:03.98 +55:05:29.8: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:26.43 +54:10:35.2: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:03.98 +55:05:29.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:48.68 +56:35:45.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:48.68 +56:35:45.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:12.04 +50:00:12.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:12.04 +50:00:12.4: 13.47 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out235420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25587.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 156s
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: 93s
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Considering the candidate 235420_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235420_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235443_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235443_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 235453_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235453_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235454_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235454_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235460_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235460_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235469_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235469_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235490_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235490_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235491_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235491_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235495_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235495_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235497_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235497_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235505_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235505_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235513_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235513_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235522_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235522_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235526_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235526_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235527_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235527_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 235538_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235538_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235539_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235539_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235548_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235548_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235560_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235560_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235563_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235563_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235582_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235582_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235583_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235583_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235585_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235585_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235599_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235599_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235602_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235602_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235608_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235608_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235615_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235615_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235616_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235616_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235617_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235617_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235622_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235622_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235630_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235630_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235633_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235633_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235635_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235635_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:21:59.37 +57:17:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235638_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235638_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235643_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235643_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:58:35.00 +54:07:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235646_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235646_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235648_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235648_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235659_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235659_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235660_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235660_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235664_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235664_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235665_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235665_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235666_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235666_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:04:36.02 +52:52:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235673_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235673_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235675_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235675_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:48:17.81 +53:25:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235679_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235679_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235681_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235681_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235688_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235688_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:08:33.54 +56:46:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235689_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235689_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235691_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235691_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:56:55.39 +55:04:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235693_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235693_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:22:17.53 +54:20:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235696_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235696_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 235698_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235698_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235700_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235700_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235702_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235702_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235708_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235708_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:27:36.43 +55:43:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235709_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235709_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235720_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235720_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235726_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235726_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235737_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235737_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235742_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235742_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235746_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235746_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235749_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235749_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235750_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235750_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:01:35.84 +53:43:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235754_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235754_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:24:56.16 +57:05:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235756_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235756_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235757_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235757_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 235760_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235760_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:11:49.51 +54:49:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235762_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235762_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:17:46.78 +55:03:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235766_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235766_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:23:58.91 +55:31:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235768_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235768_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235770_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235770_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:55:04.04 +54:11:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235775_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235775_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235776_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235776_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:29:32.13 +55:19:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235779_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235779_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235780_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235780_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:04:21.87 +51:49:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235782_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235782_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:20:24.73 +53:16:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235786_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235786_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235789_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235789_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:57:15.93 +56:30:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235791_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235791_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:06:20.97 +56:11:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235794_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235794_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235799_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235799_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235803_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235803_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235812_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235812_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235815_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235815_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235818_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235818_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235823_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235823_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 235825_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235825_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235826_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235826_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235828_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235828_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:14:15.39 +54:02:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235831_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235831_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235833_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235833_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235838_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235838_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235841_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235841_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235843_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235843_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235844_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235844_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235846_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235846_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235847_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235847_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 235850_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235850_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:51:56.60 +53:07:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235855_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235855_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235863_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235863_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235865_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235865_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235868_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235868_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:46:46.55 +51:02:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235869_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 235869_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 235955_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235955_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235990_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 235990_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236026_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236026_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236028_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236028_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 236089_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236089_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236168_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236168_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 236242_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236242_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236272_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236272_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:54:36.36 +57:28:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236299_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236299_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 236339_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236339_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:20:34.09 +52:06:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236348_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236348_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:18:49.83 +54:33:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236363_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236363_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236384_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236384_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:25:37.27 +53:21:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236405_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236405_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236414_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236414_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 236427_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236427_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236466_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236466_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236517_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236517_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236522_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236522_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:23:25.80 +55:49:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236535_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236535_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:57:59.46 +50:26:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236548_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236548_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236551_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236551_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 236555_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236555_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:43:18.26 +50:54:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236567_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236567_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:33:33.39 +52:09:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236584_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236584_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:22:51.13 +52:21:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236589_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236589_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:41:07.30 +51:33:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236613_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236613_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 236638_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236638_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:18:03.81 +49:50:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236645_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236645_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
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Considering the candidate 236660_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236660_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 236685_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236685_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:43:15.38 +51:56:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236697_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236697_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 236703_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236703_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 236712_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236712_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 236722_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236722_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
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Considering the candidate 236728_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236728_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:56:32.02 +53:44:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236735_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236735_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:58:51.59 +54:42:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236745_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236745_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236754_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236754_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:14:01.16 +55:16:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236762_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236762_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:38:44.29 +56:37:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236771_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236771_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:55:15.64 +50:14:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236781_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236781_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:29:50.19 +54:38:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236782_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236782_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:20:12.43 +50:06:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236783_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236783_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:59:00.33 +53:16:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236844_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236844_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:57:58.33 +50:27:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236856_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236856_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:27:19.28 +49:58:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236896_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236896_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:24:57.61 +53:01:57.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236906_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236906_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:40:53.46 +54:25:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236909_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236909_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236911_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236911_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236915_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236915_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236922_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236922_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:13:03.00 +49:56:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236927_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236927_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:31:40.42 +54:09:34.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236949_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236949_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:52:01.74 +50:05:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236988_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 236988_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236989_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236989_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:44:20.36 +57:20:45.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236999_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 236999_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237010_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237010_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:20:15.59 +57:50:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237016_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237016_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:02:26.93 +54:33:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237017_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237017_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237018_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237018_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:31:37.34 +56:54:57.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237025_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237025_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:22:46.41 +56:26:54.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237026_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237026_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237032_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237032_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237033_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237033_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:12:07.23 +53:36:08.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237060_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237060_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237061_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237061_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:31:16.94 +57:14:13.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237074_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237074_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:21:17.04 +55:54:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237077_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237077_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:12:36.43 +57:12:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237107_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237107_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237111_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237111_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:48:26.60 +54:40:41.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237112_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237112_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:14:16.45 +56:52:53.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237116_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237116_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237118_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237118_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:32:59.70 +57:36:34.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237129_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237129_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237140_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237140_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237146_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237146_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:56:17.39 +53:09:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237150_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237150_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237152_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237152_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:50:23.41 +54:12:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237178_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237178_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:00:26.52 +55:27:29.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237196_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237196_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:29:46.78 +54:39:58.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237212_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237212_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237216_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237216_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:19:49.04 +50:46:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237217_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237217_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237220_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237220_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237233_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237233_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:51:04.26 +51:22:54.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237235_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237235_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:24:30.56 +56:57:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237243_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237243_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237256_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237256_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:54:44.65 +53:43:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237259_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237259_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237262_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237262_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237264_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237264_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237277_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237277_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237287_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237287_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237297_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237297_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237305_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237305_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:44:44.50 +55:46:29.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237311_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237311_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237315_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237315_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237323_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237323_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237325_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237325_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237348_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237348_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:12:53.24 +55:50:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237356_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237356_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237359_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237359_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:27:21.98 +54:05:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237365_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237365_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237371_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237371_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237372_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237372_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:07:40.66 +57:11:24.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237386_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237386_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237401_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237401_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:03:41.06 +53:56:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237433_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237433_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237442_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237442_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237454_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237454_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237457_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237457_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237468_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237468_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237474_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237474_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237503_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237503_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237533_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237533_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237575_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237575_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:24:30.37 +53:19:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237583_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237583_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237604_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237604_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237630_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237630_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237632_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237632_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237648_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237648_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237651_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237651_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237659_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237659_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237661_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237661_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237681_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237681_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237708_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237708_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237710_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 237710_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237711_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 237711_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38712_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 38712_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46841_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 46841_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:09:36.44 +51:34:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219159_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 219159_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:27:11.54 +53:53:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
Preparing report for the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197606_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 197606_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:44:31.92 +56:34:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179100_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 179100_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:15:50.77 +57:32:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176581_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 176581_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 229278_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 229278_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64302_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 64302_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 00:02:27.25 +52:33:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220968_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063
The candidate 220968_fd_Cas-04-Q2b1x1_2026-07-16_22-50-33_20.00sec_4.90C_LIGHT_0063 did not pass the final checks
**** FOUND 23:44:49.25 +50:34:37.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 17s
make_report_in_HTML.sh TOTAL: 266s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:09:24.01 +54:46:43.2
00:19:34.69 +55:29:44.7
23:54:10.44 +57:04:44.9
00:04:11.10 +55:35:59.3
23:44:33.06 +53:02:41.7
00:01:47.52 +56:08:36.5
23:27:00.60 +53:39:35.5
23:43:43.11 +51:35:38.7
00:05:06.39 +54:18:27.5
00:23:01.45 +53:17:43.1
23:44:22.42 +54:06:37.2
23:45:18.41 +55:48:26.7
00:04:07.72 +56:06:31.7
00:26:43.25 +57:15:39.5
23:45:47.75 +57:16:15.6
23:40:06.44 +54:53:06.6
23:39:18.26 +52:16:23.0
00:14:34.69 +54:09:02.7
23:41:11.69 +57:06:26.0
23:42:48.94 +51:38:41.5
00:25:31.28 +56:42:26.6
23:23:51.26 +49:17:44.6
00:17:02.06 +57:24:19.4
00:15:18.03 +53:07:47.9
23:50:03.35 +50:48:21.6
23:21:10.53 +53:55:05.7
23:41:09.34 +52:19:40.5
23:46:38.90 +53:36:25.0
00:31:00.11 +57:25:00.4
23:17:04.21 +54:39:05.3
23:57:18.96 +54:52:41.6
23:38:57.63 +54:45:08.9
23:32:25.66 +51:54:37.0
00:19:05.99 +56:05:26.7
23:39:31.70 +55:18:15.4
23:36:55.82 +54:03:11.7
00:25:59.36 +55:56:51.7
00:10:28.24 +51:50:29.5
23:28:57.54 +51:01:11.3
23:41:28.17 +52:04:54.8
23:30:17.84 +54:52:52.7
23:14:01.73 +55:14:39.2
23:15:56.67 +52:27:19.8
23:14:53.64 +56:49:23.2
23:18:18.47 +56:19:03.0
00:06:20.74 +54:44:20.6
23:58:38.58 +53:54:04.6
00:30:31.18 +55:56:24.5
23:13:06.15 +53:45:12.2
00:19:09.98 +52:36:33.5
23:18:56.70 +53:20:37.3
23:12:41.18 +54:49:13.0
23:10:02.58 +56:51:40.1
23:46:36.45 +51:42:14.5
00:13:40.71 +56:53:48.4
23:20:46.33 +53:39:16.9
00:24:24.45 +57:11:31.3
23:33:10.46 +52:52:20.6
00:15:19.54 +53:12:02.4
23:15:52.58 +52:57:58.3
23:43:27.95 +50:54:08.4
23:12:17.67 +57:05:09.0
23:25:27.95 +49:20:12.5
23:26:01.34 +49:55:47.2
00:14:30.86 +56:43:29.5
23:33:41.01 +49:58:07.5
23:41:50.01 +54:40:26.7
23:34:08.29 +54:02:58.4
23:21:05.80 +55:55:39.5
23:24:53.16 +54:29:06.1
23:11:51.35 +55:18:28.6
23:29:18.29 +50:38:17.6
23:28:27.72 +53:49:29.8
23:58:30.70 +56:50:31.0
00:11:12.46 +57:36:24.6
23:49:51.83 +52:07:56.1
00:04:53.61 +51:59:42.5
23:28:08.32 +53:01:02.4
23:16:57.02 +54:01:33.6
23:32:21.35 +53:10:39.0
23:26:28.94 +53:45:56.0
23:14:46.41 +54:27:10.1
00:10:04.53 +50:47:22.2
23:31:29.93 +54:52:04.1
00:03:26.43 +54:10:35.2
23:49:03.98 +55:05:29.8
00:03:48.68 +56:35:45.5
23:21:12.04 +50:00:12.4
########### Completed Cas-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
00:09:24.01 +54:46:43.2
00:19:34.69 +55:29:44.7
23:54:10.44 +57:04:44.9
00:04:11.10 +55:35:59.3
23:44:33.06 +53:02:41.7
00:01:47.52 +56:08:36.5
23:27:00.60 +53:39:35.5
23:43:43.11 +51:35:38.7
00:05:06.39 +54:18:27.5
00:23:01.45 +53:17:43.1
23:44:22.42 +54:06:37.2
23:45:18.41 +55:48:26.7
00:04:07.72 +56:06:31.7
00:26:43.25 +57:15:39.5
23:45:47.75 +57:16:15.6
23:40:06.44 +54:53:06.6
23:39:18.26 +52:16:23.0
00:14:34.69 +54:09:02.7
23:41:11.69 +57:06:26.0
23:42:48.94 +51:38:41.5
00:25:31.28 +56:42:26.6
23:23:51.26 +49:17:44.6
00:17:02.06 +57:24:19.4
00:15:18.03 +53:07:47.9
23:50:03.35 +50:48:21.6
23:21:10.53 +53:55:05.7
23:41:09.34 +52:19:40.5
23:46:38.90 +53:36:25.0
00:31:00.11 +57:25:00.4
23:17:04.21 +54:39:05.3
23:57:18.96 +54:52:41.6
23:38:57.63 +54:45:08.9
23:32:25.66 +51:54:37.0
00:19:05.99 +56:05:26.7
23:39:31.70 +55:18:15.4
23:36:55.82 +54:03:11.7
00:25:59.36 +55:56:51.7
00:10:28.24 +51:50:29.5
23:28:57.54 +51:01:11.3
23:41:28.17 +52:04:54.8
23:30:17.84 +54:52:52.7
23:14:01.73 +55:14:39.2
23:15:56.67 +52:27:19.8
23:14:53.64 +56:49:23.2
23:18:18.47 +56:19:03.0
00:06:20.74 +54:44:20.6
23:58:38.58 +53:54:04.6
00:30:31.18 +55:56:24.5
23:13:06.15 +53:45:12.2
00:19:09.98 +52:36:33.5
23:18:56.70 +53:20:37.3
23:12:41.18 +54:49:13.0
23:10:02.58 +56:51:40.1
23:46:36.45 +51:42:14.5
00:13:40.71 +56:53:48.4
23:20:46.33 +53:39:16.9
00:24:24.45 +57:11:31.3
23:33:10.46 +52:52:20.6
00:15:19.54 +53:12:02.4
23:15:52.58 +52:57:58.3
23:43:27.95 +50:54:08.4
23:12:17.67 +57:05:09.0
23:25:27.95 +49:20:12.5
23:26:01.34 +49:55:47.2
00:14:30.86 +56:43:29.5
23:33:41.01 +49:58:07.5
23:41:50.01 +54:40:26.7
23:34:08.29 +54:02:58.4
23:21:05.80 +55:55:39.5
23:24:53.16 +54:29:06.1
23:11:51.35 +55:18:28.6
23:29:18.29 +50:38:17.6
23:28:27.72 +53:49:29.8
23:58:30.70 +56:50:31.0
00:11:12.46 +57:36:24.6
23:49:51.83 +52:07:56.1
00:04:53.61 +51:59:42.5
23:28:08.32 +53:01:02.4
23:16:57.02 +54:01:33.6
23:32:21.35 +53:10:39.0
23:26:28.94 +53:45:56.0
23:14:46.41 +54:27:10.1
00:10:04.53 +50:47:22.2
23:31:29.93 +54:52:04.1
00:03:26.43 +54:10:35.2
23:49:03.98 +55:05:29.8
00:03:48.68 +56:35:45.5
23:21:12.04 +50:00:12.4
###################################################################################
00:09:24.01 +54:46:43.2 -- not an asteroid (will add it to exclusion list)
00:19:34.69 +55:29:44.7 -- not an asteroid (will add it to exclusion list)
23:54:10.44 +57:04:44.9 -- not an asteroid (will add it to exclusion list)
00:04:11.10 +55:35:59.3 -- not an asteroid (will add it to exclusion list)
23:44:33.06 +53:02:41.7 -- not an asteroid (will add it to exclusion list)
00:01:47.52 +56:08:36.5 -- not an asteroid (will add it to exclusion list)
23:27:00.60 +53:39:35.5 -- not an asteroid (will add it to exclusion list)
23:43:43.11 +51:35:38.7 -- not an asteroid (will add it to exclusion list)
00:05:06.39 +54:18:27.5 -- not an asteroid (will add it to exclusion list)
00:23:01.45 +53:17:43.1 -- not an asteroid (will add it to exclusion list)
23:44:22.42 +54:06:37.2 -- not an asteroid (will add it to exclusion list)
23:45:18.41 +55:48:26.7 -- not an asteroid (will add it to exclusion list)
00:04:07.72 +56:06:31.7 -- not an asteroid (will add it to exclusion list)
00:26:43.25 +57:15:39.5 -- not an asteroid (will add it to exclusion list)
23:45:47.75 +57:16:15.6 -- not an asteroid (will add it to exclusion list)
23:40:06.44 +54:53:06.6 -- not an asteroid (will add it to exclusion list)
23:39:18.26 +52:16:23.0 -- not an asteroid (will add it to exclusion list)
00:14:34.69 +54:09:02.7 -- not an asteroid (will add it to exclusion list)
23:41:11.69 +57:06:26.0 -- not an asteroid (will add it to exclusion list)
23:42:48.94 +51:38:41.5 -- not an asteroid (will add it to exclusion list)
00:25:31.28 +56:42:26.6 -- not an asteroid (will add it to exclusion list)
23:23:51.26 +49:17:44.6 -- not an asteroid (will add it to exclusion list)
00:17:02.06 +57:24:19.4 -- not an asteroid (will add it to exclusion list)
00:15:18.03 +53:07:47.9 -- not an asteroid (will add it to exclusion list)
23:50:03.35 +50:48:21.6 -- not an asteroid (will add it to exclusion list)
23:21:10.53 +53:55:05.7 -- not an asteroid (will add it to exclusion list)
23:41:09.34 +52:19:40.5 -- not an asteroid (will add it to exclusion list)
23:46:38.90 +53:36:25.0 -- not an asteroid (will add it to exclusion list)
00:31:00.11 +57:25:00.4 -- not an asteroid (will add it to exclusion list)
23:17:04.21 +54:39:05.3 -- not an asteroid (will add it to exclusion list)
23:57:18.96 +54:52:41.6 -- not an asteroid (will add it to exclusion list)
23:38:57.63 +54:45:08.9 -- not an asteroid (will add it to exclusion list)
23:32:25.66 +51:54:37.0 -- not an asteroid (will add it to exclusion list)
00:19:05.99 +56:05:26.7 -- not an asteroid (will add it to exclusion list)
23:39:31.70 +55:18:15.4 -- not an asteroid (will add it to exclusion list)
23:36:55.82 +54:03:11.7 -- not an asteroid (will add it to exclusion list)
00:25:59.36 +55:56:51.7 -- not an asteroid (will add it to exclusion list)
00:10:28.24 +51:50:29.5 -- not an asteroid (will add it to exclusion list)
23:28:57.54 +51:01:11.3 -- not an asteroid (will add it to exclusion list)
23:41:28.17 +52:04:54.8 -- not an asteroid (will add it to exclusion list)
23:30:17.84 +54:52:52.7 -- not an asteroid (will add it to exclusion list)
23:14:01.73 +55:14:39.2 -- not an asteroid (will add it to exclusion list)
23:15:56.67 +52:27:19.8 -- not an asteroid (will add it to exclusion list)
23:14:53.64 +56:49:23.2 -- not an asteroid (will add it to exclusion list)
23:18:18.47 +56:19:03.0 -- not an asteroid (will add it to exclusion list)
00:06:20.74 +54:44:20.6 -- not an asteroid (will add it to exclusion list)
23:58:38.58 +53:54:04.6 -- not an asteroid (will add it to exclusion list)
00:30:31.18 +55:56:24.5 -- not an asteroid (will add it to exclusion list)
23:13:06.15 +53:45:12.2 -- not an asteroid (will add it to exclusion list)
00:19:09.98 +52:36:33.5 -- not an asteroid (will add it to exclusion list)
23:18:56.70 +53:20:37.3 -- not an asteroid (will add it to exclusion list)
23:12:41.18 +54:49:13.0 -- not an asteroid (will add it to exclusion list)
23:10:02.58 +56:51:40.1 -- not an asteroid (will add it to exclusion list)
23:46:36.45 +51:42:14.5 -- not an asteroid (will add it to exclusion list)
00:13:40.71 +56:53:48.4 -- not an asteroid (will add it to exclusion list)
23:20:46.33 +53:39:16.9 -- not an asteroid (will add it to exclusion list)
00:24:24.45 +57:11:31.3 -- not an asteroid (will add it to exclusion list)
23:33:10.46 +52:52:20.6 -- not an asteroid (will add it to exclusion list)
00:15:19.54 +53:12:02.4 -- not an asteroid (will add it to exclusion list)
23:15:52.58 +52:57:58.3 -- not an asteroid (will add it to exclusion list)
23:43:27.95 +50:54:08.4 -- not an asteroid (will add it to exclusion list)
23:12:17.67 +57:05:09.0 -- not an asteroid (will add it to exclusion list)
23:25:27.95 +49:20:12.5 -- not an asteroid (will add it to exclusion list)
23:26:01.34 +49:55:47.2 -- not an asteroid (will add it to exclusion list)
00:14:30.86 +56:43:29.5 -- not an asteroid (will add it to exclusion list)
23:33:41.01 +49:58:07.5 -- not an asteroid (will add it to exclusion list)
23:41:50.01 +54:40:26.7 -- not an asteroid (will add it to exclusion list)
23:34:08.29 +54:02:58.4 -- not an asteroid (will add it to exclusion list)
23:21:05.80 +55:55:39.5 -- not an asteroid (will add it to exclusion list)
23:24:53.16 +54:29:06.1 -- not an asteroid (will add it to exclusion list)
23:11:51.35 +55:18:28.6 -- not an asteroid (will add it to exclusion list)
23:29:18.29 +50:38:17.6 -- not an asteroid (will add it to exclusion list)
23:28:27.72 +53:49:29.8 -- not an asteroid (will add it to exclusion list)
23:58:30.70 +56:50:31.0 -- not an asteroid (will add it to exclusion list)
00:11:12.46 +57:36:24.6 -- not an asteroid (will add it to exclusion list)
23:49:51.83 +52:07:56.1 -- not an asteroid (will add it to exclusion list)
00:04:53.61 +51:59:42.5 -- not an asteroid (will add it to exclusion list)
23:28:08.32 +53:01:02.4 -- not an asteroid (will add it to exclusion list)
23:16:57.02 +54:01:33.6 -- not an asteroid (will add it to exclusion list)
23:32:21.35 +53:10:39.0 -- not an asteroid (will add it to exclusion list)
23:26:28.94 +53:45:56.0 -- not an asteroid (will add it to exclusion list)
23:14:46.41 +54:27:10.1 -- not an asteroid (will add it to exclusion list)
00:10:04.53 +50:47:22.2 -- not an asteroid (will add it to exclusion list)
23:31:29.93 +54:52:04.1 -- not an asteroid (will add it to exclusion list)
00:03:26.43 +54:10:35.2 -- not an asteroid (will add it to exclusion list)
23:49:03.98 +55:05:29.8 -- not an asteroid (will add it to exclusion list)
00:03:48.68 +56:35:45.5 -- not an asteroid (will add it to exclusion list)
23:21:12.04 +50:00:12.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:01:47.52 +56:08:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:26.43 +54:10:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:48.68 +56:35:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:07.72 +56:06:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:11.10 +55:35:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:53.61 +51:59:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:06.39 +54:18:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:20.74 +54:44:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:24.01 +54:46:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:04.53 +50:47:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:28.24 +51:50:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:12.46 +57:36:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:40.71 +56:53:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:30.86 +56:43:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:34.69 +54:09:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:18.03 +53:07:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:19.54 +53:12:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:02.06 +57:24:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:05.99 +56:05:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:09.98 +52:36:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:34.69 +55:29:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:01.45 +53:17:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:24.45 +57:11:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:31.28 +56:42:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:59.36 +55:56:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:43.25 +57:15:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:31.18 +55:56:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:00.11 +57:25:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:02.58 +56:51:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:51.35 +55:18:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:17.67 +57:05:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:41.18 +54:49:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:06.15 +53:45:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:01.73 +55:14:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:46.41 +54:27:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:53.64 +56:49:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:52.58 +52:57:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:56.67 +52:27:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:57.02 +54:01:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:04.21 +54:39:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:18.47 +56:19:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:56.70 +53:20:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:46.33 +53:39:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:05.80 +55:55:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:10.53 +53:55:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:12.04 +50:00:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:51.26 +49:17:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:53.16 +54:29:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:27.95 +49:20:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:01.34 +49:55:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:28.94 +53:45:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:00.60 +53:39:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:08.32 +53:01:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:27.72 +53:49:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:57.54 +51:01:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:18.29 +50:38:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:17.84 +54:52:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:29.93 +54:52:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:21.35 +53:10:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:25.66 +51:54:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:10.46 +52:52:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:41.01 +49:58:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:08.29 +54:02:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:55.82 +54:03:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:57.63 +54:45:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:18.26 +52:16:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:31.70 +55:18:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:06.44 +54:53:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:09.34 +52:19:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:11.69 +57:06:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:28.17 +52:04:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:50.01 +54:40:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:48.94 +51:38:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:27.95 +50:54:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:43.11 +51:35:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:22.42 +54:06:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:33.06 +53:02:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:18.41 +55:48:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:47.75 +57:16:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:36.45 +51:42:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:38.90 +53:36:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:03.98 +55:05:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:51.83 +52:07:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:03.35 +50:48:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:10.44 +57:04:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:18.96 +54:52:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:30.70 +56:50:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:38.58 +53:54:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:01:47.52 +56:08:36.5 -- not a known variable star
00:03:26.43 +54:10:35.2 -- not a known variable star
00:03:48.68 +56:35:45.5 -- not a known variable star
00:04:07.72 +56:06:31.7 -- not a known variable star
00:04:11.10 +55:35:59.3 -- not a known variable star
00:04:53.61 +51:59:42.5 -- not a known variable star
00:05:06.39 +54:18:27.5 -- a known variable star
00:06:20.74 +54:44:20.6 -- not a known variable star
00:09:24.01 +54:46:43.2 -- not a known variable star
00:10:04.53 +50:47:22.2 -- not a known variable star
00:10:28.24 +51:50:29.5 -- not a known variable star
00:11:12.46 +57:36:24.6 -- not a known variable star
00:13:40.71 +56:53:48.4 -- not a known variable star
00:14:30.86 +56:43:29.5 -- not a known variable star
00:14:34.69 +54:09:02.7 -- not a known variable star
00:15:18.03 +53:07:47.9 -- a known variable star
00:15:19.54 +53:12:02.4 -- a known variable star
00:17:02.06 +57:24:19.4 -- not a known variable star
00:19:05.99 +56:05:26.7 -- not a known variable star
00:19:09.98 +52:36:33.5 -- not a known variable star
00:19:34.69 +55:29:44.7 -- a known variable star
00:23:01.45 +53:17:43.1 -- not a known variable star
00:24:24.45 +57:11:31.3 -- a known variable star
00:25:31.28 +56:42:26.6 -- not a known variable star
00:25:59.36 +55:56:51.7 -- a known variable star
00:26:43.25 +57:15:39.5 -- not a known variable star
00:30:31.18 +55:56:24.5 -- a known variable star
00:31:00.11 +57:25:00.4 -- a known variable star
23:10:02.58 +56:51:40.1 -- not a known variable star
23:11:51.35 +55:18:28.6 -- a known variable star
23:12:17.67 +57:05:09.0 -- not a known variable star
23:12:41.18 +54:49:13.0 -- not a known variable star
23:13:06.15 +53:45:12.2 -- a known variable star
23:14:01.73 +55:14:39.2 -- not a known variable star
23:14:46.41 +54:27:10.1 -- not a known variable star
23:14:53.64 +56:49:23.2 -- a known variable star
23:15:52.58 +52:57:58.3 -- not a known variable star
23:15:56.67 +52:27:19.8 -- not a known variable star
23:16:57.02 +54:01:33.6 -- a known variable star
23:17:04.21 +54:39:05.3 -- a known variable star
23:18:18.47 +56:19:03.0 -- not a known variable star
23:18:56.70 +53:20:37.3 -- a known variable star
23:20:46.33 +53:39:16.9 -- a known variable star
23:21:05.80 +55:55:39.5 -- not a known variable star
23:21:10.53 +53:55:05.7 -- not a known variable star
23:21:12.04 +50:00:12.4 -- a known variable star
23:23:51.26 +49:17:44.6 -- not a known variable star
23:24:53.16 +54:29:06.1 -- not a known variable star
23:25:27.95 +49:20:12.5 -- not a known variable star
23:26:01.34 +49:55:47.2 -- a known variable star
23:26:28.94 +53:45:56.0 -- not a known variable star
23:27:00.60 +53:39:35.5 -- not a known variable star
23:28:08.32 +53:01:02.4 -- not a known variable star
23:28:27.72 +53:49:29.8 -- not a known variable star
23:28:57.54 +51:01:11.3 -- not a known variable star
23:29:18.29 +50:38:17.6 -- not a known variable star
23:30:17.84 +54:52:52.7 -- not a known variable star
23:31:29.93 +54:52:04.1 -- not a known variable star
23:32:21.35 +53:10:39.0 -- not a known variable star
23:32:25.66 +51:54:37.0 -- a known variable star
23:33:10.46 +52:52:20.6 -- not a known variable star
23:33:41.01 +49:58:07.5 -- not a known variable star
23:34:08.29 +54:02:58.4 -- a known variable star
23:36:55.82 +54:03:11.7 -- not a known variable star
23:38:57.63 +54:45:08.9 -- not a known variable star
23:39:18.26 +52:16:23.0 -- not a known variable star
23:39:31.70 +55:18:15.4 -- not a known variable star
23:40:06.44 +54:53:06.6 -- not a known variable star
23:41:09.34 +52:19:40.5 -- not a known variable star
23:41:11.69 +57:06:26.0 -- not a known variable star
23:41:28.17 +52:04:54.8 -- not a known variable star
23:41:50.01 +54:40:26.7 -- not a known variable star
23:42:48.94 +51:38:41.5 -- a known variable star
23:43:27.95 +50:54:08.4 -- a known variable star
23:43:43.11 +51:35:38.7 -- not a known variable star
23:44:22.42 +54:06:37.2 -- not a known variable star
23:44:33.06 +53:02:41.7 -- not a known variable star
23:45:18.41 +55:48:26.7 -- not a known variable star
23:45:47.75 +57:16:15.6 -- not a known variable star
23:46:36.45 +51:42:14.5 -- not a known variable star
23:46:38.90 +53:36:25.0 -- not a known variable star
23:49:03.98 +55:05:29.8 -- not a known variable star
23:49:51.83 +52:07:56.1 -- a known variable star
23:50:03.35 +50:48:21.6 -- not a known variable star
23:54:10.44 +57:04:44.9 -- not a known variable star
23:57:18.96 +54:52:41.6 -- a known variable star
23:58:30.70 +56:50:31.0 -- not a known variable star
23:58:38.58 +53:54:04.6 -- not a known variable star
Found 65 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
88 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 88 (excluding asteroids and hot pixels, 65 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)2461238.65976169 -observatory V36
07:14:46.68 +17:23:04.8 Mercury (4.5mag)
10:39:37.67 +09:36:35.5 Venus (-4.2mag)
04:44:21.24 +22:11:39.7 Mars (1.3mag)
08:22:52.52 +19:51:32.4 Jupiter (-1.8mag)
00:56:27.29 +03:22:13.1 Saturn (0.7mag)
04:08:29.24 +20:48:25.4 Uranus (5.8mag)
00:16:56.90 +00:19:48.2 Neptune (7.7mag)
20:30:16.70 -23:21:00.1 Pluto (14.4mag)
10:11:37.42 +10:07:49.6 Moon (-9.0mag)
-rw-r--r-- 1 apache apache 361 Jul 16 22:58 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461238.65976169:
08:22:54.01 +19:51:28.7 Io (6.0mag)
08:22:50.02 +19:51:43.6 Europa (6.3mag)
08:23:07.37 +19:50:37.7 Ganymede (5.6mag)
08:22:26.42 +19:53:10.9 Callisto (6.8mag)
08:21:06.03 +19:38:43.5 Himalia (15.7mag)
08:22:53.53 +19:51:29.0 Thebe (16.6mag)
08:20:26.88 +19:41:41.6 Elara (17.7mag)
08:26:36.58 +19:42:05.0 Pasiphae (17.9mag)
08:27:26.66 +19:57:38.8 Carme (19.0mag)
00:56:39.32 +03:22:07.8 Titan (8.5mag)
00:56:32.35 +03:22:07.3 Rhea (9.8mag)
00:55:52.54 +03:20:12.3 Iapetus (11.2mag)
00:56:13.38 +03:22:16.2 Hyperion (14.5mag)
00:56:18.92 +03:18:27.5 Phoebe (16.5mag)
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461238.65976169:
17:57:20.01 -31:23:14.6 JWST
19:34:22.99 +04:32:26.8 Chandra
08:43:49.89 -48:43:45.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 16 22:58 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461238.65976169 -observatory V36
02:45:48.38 +15:13:00.5 17.8mag P/1996 R2 (Lagerkvist)
18:12:55.25 -34:31:25.3 13.8mag P/2010 H2 (Vales)
06:32:28.13 -68:15:42.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:08.20 +32:33:54.2 17.6mag C/2017 K2 (PANSTARRS)
02:23:04.31 +19:45:08.1 15.7mag P/2021 N1 (ZTF)
22:55:15.37 +32:14:25.1 17.3mag C/2022 E2 (ATLAS)
06:20:05.86 +26:51:34.1 16.7mag C/2022 N2 (PANSTARRS)
10:01:29.76 +29:28:28.3 16.9mag C/2022 QE78 (ATLAS)
09:14:09.61 +05:07:01.2 17.9mag C/2022 R6 (PANSTARRS)
18:03:10.54 +21:00:20.4 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:05.19 -11:33:18.4 17.8mag P/2023 B1 (PANSTARRS)
21:40:43.76 +67:30:57.8 17.8mag C/2023 H5 (Lemmon)
16:18:07.24 -10:47:00.8 14.0mag C/2023 R1 (PANSTARRS)
08:12:37.45 +66:05:07.0 17.9mag C/2024 A1 (ATLAS)
07:41:37.50 +30:20:29.6 14.8mag C/2024 E1 (Wierzchos)
15:13:15.31 +15:28:53.9 17.6mag C/2024 G6 (ATLAS)
19:32:28.36 +40:38:02.9 13.7mag C/2024 J3 (ATLAS)
21:40:10.77 +46:59:01.0 17.8mag C/2024 R4 (PANSTARRS)
04:56:00.13 -13:30:36.8 15.7mag C/2024 T5 (ATLAS)
06:40:07.63 +27:55:56.9 18.0mag C/2025 J1 (Borisov)
07:18:56.78 -13:31:26.2 16.8mag C/2025 R3 (PANSTARRS)
10:04:08.77 +22:07:52.5 17.6mag C/2025 V2 (Rankin)
12:47:04.85 +03:37:45.4 17.1mag C/2025 Y1 (ATLAS)
16:33:44.64 +79:08:55.4 17.2mag C/2026 A2 (Bok)
02:53:05.95 +45:31:20.2 16.8mag C/2026 B2 (Sun-Gao)
11:29:59.99 +05:41:33.1 17.0mag A/2026 E1
21:29:30.90 -17:39:38.5 7.1mag 10P/Tempel
11:16:44.87 -02:11:30.4 16.2mag 29P/Schwassmann-Wachmann
04:09:53.76 +30:16:55.0 17.9mag 47P/Ashbrook-Jackson
10:22:16.31 +11:49:52.6 17.1mag 63P/Wild
00:51:01.77 -05:02:46.8 15.5mag 65P/Gunn
04:43:49.39 +20:29:13.7 13.7mag 78P/Gehrels
02:33:01.00 +11:30:31.3 16.3mag 88P/Howell
06:55:35.06 +30:04:22.4 15.8mag 93P/Lovas
04:43:14.40 +31:19:10.6 16.7mag 114P/Wiseman-Skiff
08:25:19.39 +29:54:22.8 15.2mag 123P/West-Hartley
11:00:54.23 -01:34:21.2 16.9mag 124P/Mrkos
05:02:37.15 +20:59:13.5 16.2mag 128P/Shoemaker-Holt
05:49:01.33 +19:37:59.6 17.8mag 131P/Mueller
07:37:56.03 +15:30:43.0 16.4mag 141P-D/Machholz
03:19:26.40 -20:34:01.4 15.1mag 161P/Hartley-IRAS
05:57:37.64 +35:18:10.8 15.4mag 162P/SidingSpring
18:43:39.44 +19:39:44.8 14.1mag 169P/NEAT
01:57:02.21 +08:18:24.0 17.6mag 220P/McNaught
16:35:30.73 -08:41:13.6 17.2mag 235P/LINEAR
08:59:32.60 +32:39:07.6 18.0mag 240P/NEAT
20:38:39.87 -50:56:54.9 17.8mag 259P/Garradd
02:18:28.04 +15:16:31.7 15.6mag 260P/McNaught
05:57:57.52 +37:19:25.8 17.4mag 295P/LINEAR
15:06:30.84 +05:25:53.5 17.6mag 391P/Kowalski
08:40:44.63 +19:23:38.7 17.9mag 450P/LONEOS
08:02:24.47 +38:38:46.8 18.0mag 493P/LONEOS
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:33:53.06 -07:15:00.80 ASASSN-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -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
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
19:33:53.06 -07:15:00.80 2026-07-14.15 15.5
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
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:27:50.004 -06:44:08.56 AT 2026svd 2026-06-26.40 23.3852
04:22:38.209 -47:20:55.00 AT 2026svc 2026-06-26.43 22.5609
21:50:00.261 -07:57:05.98 AT 2026svb 2026-06-26.41 23.0326
00:44:37.185 -43:22:31.83 AT 2026sva 2026-06-26.42 21.6706
21:35:19.036 -19:34:24.34 AT 2026suz 2026-06-26.41 23.3439
22:40:47.013 -09:25:04.67 AT 2026suy 2026-06-26.40 23.289
22:05:53.553 -08:24:29.60 AT 2026sux 2026-06-26.41 22.2593
22:33:25.333 -02:10:00.75 AT 2026suw 2026-06-26.40 22.6919
22:01:05.082 -07:26:52.26 AT 2026suv 2026-06-26.41 22.9876
22:30:12.816 -04:52:34.67 AT 2026suu 2026-06-26.40 21.9579
21:54:55.644 -07:45:32.24 AT 2026sut 2026-06-26.41 21.0171
18:17:40.907 -50:01:40.94 AT 2026sus 2026-07-07.95 19.363
20:17:07.701 -31:44:39.62 SN 2026sur 2026-07-08.18 19.091
03:21:24.733 -45:31:36.65 AT 2026suq 2026-07-08.14 18.759
21:15:50.298 -66:09:30.96 AT 2026sup 2026-07-07.05 18.911
22:32:27.822 -20:22:41.23 AT 2026suo 2026-07-06.46 19.8035
04:03:27.102 -57:43:47.16 AT 2026sun 2026-07-08.15 18.325
23:58:57.947 -03:02:20.39 AT 2026sum 2026-07-08.38 19.6555
00:36:59.677 +43:01:07.64 AT 2026sul 2026-07-05.38 20.0025
14:33:14.800 +42:54:37.00 AT 2026suk 2026-06-30.71 21.4
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