This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy
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 22.1814 2461243.6814 12.44 23:43:36.04 +52:28:00.5
112.56580 -9.03425 galactic Cas Second-epoch detections are separated by 1.1" and 6.3 pix
The object was found in VSX21" Gaia DR3 1944978658716880512
Type: VAR
# Max. Min./Amp. JD0 Period
15.180 G 15.260 G 0.024879600000 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 23:43:36.04 +52:28:00.5: 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 23:43:36.04 +52:28:00.5: 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 22.1814* 23 43 36.04 +52 28 00.5 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 1944978658716880512,2461243.6814,12.44,0.05,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 1944978658716880512 20260722.1814 12.44CV 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 22.1814 2461243.6814 12.31 23:53:54.31 +51:24:50.5
113.86796 -10.44238 galactic Cas Second-epoch detections are separated by 3.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J358.4667+51.4085 | 23:53:54.31 +51:24:50.5 (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 23:53:54.31 +51:24:50.5: 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 23:53:54.31 +51:24:50.5: 13.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 53 54.31 +51 24 50.5 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
ATO J358.4667+51.4085,2461243.6814,12.31,0.05,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
ATO J358.4667+51.4085 20260722.1814 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 22.1814 2461243.6814 12.01 00:12:16.50 +51:27:00.4
116.73536 -10.94984 galactic Cas Second-epoch detections are separated by 3.0" and 5.9 pix
The object was found in VSX 3" Gaia DR3 395759697073934848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.860 G 13.900 G 0.107054100000 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 00:12:16.50 +51:27:00.4: 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 00:12:16.50 +51:27:00.4: 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 22.1814* 00 12 16.50 +51 27 00.4 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 395759697073934848,2461243.6814,12.01,0.05,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
Gaia DR3 395759697073934848 20260722.1814 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 22.1814 2461243.6814 12.20 23:41:11.48 +57:06:44.9
113.47324 -4.46361 galactic Cas Second-epoch detections are separated by 1.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.3012+57.1115 | 23:41:11.48 +57:06:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:11.48 +57:06:44.9: 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 23:41:11.48 +57:06:44.9: 13.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 41 11.48 +57 06 44.9 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
ATO J355.3012+57.1115,2461243.6814,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.3012+57.1115 20260722.1814 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 12.15 00:04:07.71 +56:06:31.4
116.33094 -6.15549 galactic Cas Second-epoch detections are separated by 2.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.0225+56.1167 | 00:04:07.71 +56:06:31.4 (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 00:04:07.71 +56:06:31.4: 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 00:04:07.71 +56:06:31.4: 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 22.1814* 00 04 07.71 +56 06 31.4 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
ATO J001.0225+56.1167,2461243.6814,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.0225+56.1167 20260722.1814 12.15CV 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 22.1814 2461243.6814 12.29 23:23:45.48 +55:35:38.4
110.70367 -5.18222 galactic Cas Second-epoch detections are separated by 2.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.9400+55.5976 | 23:23:45.48 +55:35:38.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.730+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:45.48 +55:35:38.4: 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 23:23:45.48 +55:35:38.4: 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 22.1814* 23 23 45.48 +55 35 38.4 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
ATO J350.9400+55.5976,2461243.6814,12.29,0.05,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 J350.9400+55.5976 20260722.1814 12.29CV 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 22.1814 2461243.6814 12.22 23:43:58.89 +55:38:49.6
113.45810 -5.97892 galactic Cas Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:43:58.89 +55:38:49.6 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:58.89 +55:38:49.6: 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 23:43:58.89 +55:38:49.6: 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 22.1814* 23 43 58.89 +55 38 49.6 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
target,2461243.6814,12.22,0.05,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 20260722.1814 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 22.1814 2461243.6814 12.03 00:01:47.63 +56:08:37.0
116.01619 -6.06010 galactic Cas Second-epoch detections are separated by 0.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:01:47.63 +56:08:37.0 (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 00:01:47.63 +56:08:37.0: 13.63 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:47.63 +56:08:37.0: 13.17 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 00 01 47.63 +56 08 37.0 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,2461243.6814,12.03,0.05,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
target 20260722.1814 12.03CV 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 22.1814 2461243.6814 12.11 00:07:14.46 +56:13:57.1
116.78181 -6.11055 galactic Cas Second-epoch detections are separated by 2.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 420957995321025152 | 00:07:11.30 +56:14:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.369+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:14.46 +56:13:57.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:14.46 +56:13:57.1: 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 22.1814* 00 07 14.46 +56 13 57.1 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 420957995321025152,2461243.6814,12.11,0.05,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
Gaia DR3 420957995321025152 20260722.1814 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 22.1814 2461243.6814 12.15 23:46:15.08 +52:45:11.3
113.03411 -8.86135 galactic Cas Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1945363281626831488 | 23:46:14.29 +52:44:50.1 (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 23:46:15.08 +52:45:11.3: 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 23:46:15.08 +52:45:11.3: 13.67 +/- 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 22.1814* 23 46 15.08 +52 45 11.3 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
Gaia DR3 1945363281626831488,2461243.6814,12.15,0.05,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 1945363281626831488 20260722.1814 12.15CV 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 22.1814 2461243.6814 11.99 23:40:15.74 +52:16:46.3
112.01785 -9.07748 galactic Cas Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:40:15.74 +52:16:46.3 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.036 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:40:15.74 +52:16:46.3: 13.59 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:40:15.74 +52:16:46.3: 13.29 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 40 15.74 +52 16 46.3 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461243.6814,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260722.1814 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 12.11 23:45:47.77 +57:16:14.9
114.11866 -4.47343 galactic Cas Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.4612+57.2675 | 23:45:47.77 +57:16:14.9 (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 23:45:47.77 +57:16:14.9: 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 23:45:47.77 +57:16:14.9: 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 22.1814* 23 45 47.77 +57 16 14.9 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+57.2675,2461243.6814,12.11,0.05,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 J356.4612+57.2675 20260722.1814 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 22.1814 2461243.6814 11.98 23:31:48.19 +56:54:17.7
112.18570 -4.29605 galactic Cas Second-epoch detections are separated by 0.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1998596652484201600 | 23:31:48.61 +56:53:39.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.415+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:48.19 +56:54:17.7: 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 23:31:48.19 +56:54:17.7: 13.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 31 48.19 +56 54 17.7 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
Gaia DR3 1998596652484201600,2461243.6814,11.98,0.05,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 1998596652484201600 20260722.1814 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 12.01 23:37:08.58 +50:09:11.0
110.93279 -10.97979 galactic And Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1943714387842598272 | 23:37:06.16 +50:09:37.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.339+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:08.58 +50:09:11.0: 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 23:37:08.58 +50:09:11.0: 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 22.1814* 23 37 08.58 +50 09 11.0 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943714387842598272,2461243.6814,12.01,0.05,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
Gaia DR3 1943714387842598272 20260722.1814 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 22.1814 2461243.6814 11.96 23:44:34.18 +53:02:54.6
112.86255 -8.51094 galactic Cas Second-epoch detections are separated by 1.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:44:34.18 +53:02:54.6 (user input) | T | P | (position from user input) J-Ks=0.466+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:34.18 +53:02:54.6: 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 23:44:34.18 +53:02:54.6: 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 22.1814* 23 44 34.18 +53 02 54.6 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,2461243.6814,11.96,0.05,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
target 20260722.1814 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 22.1814 2461243.6814 11.81 23:47:35.26 +55:28:20.1
113.90974 -6.27705 galactic Cas Second-epoch detections are separated by 1.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:47:35.26 +55:28:20.1 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:35.26 +55:28:20.1: 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 23:47:35.26 +55:28:20.1: 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 22.1814* 23 47 35.26 +55 28 20.1 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,2461243.6814,11.81,0.05,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
target 20260722.1814 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 22.1814 2461243.6814 11.85 23:39:31.92 +55:18:14.6
112.75486 -6.14050 galactic Cas Second-epoch detections are separated by 1.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:39:31.92 +55:18:14.6 (user input) | T | P | (position from user input) 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 23:39:31.92 +55:18:14.6: 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 23:39:31.92 +55:18:14.6: 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 22.1814* 23 39 31.92 +55 18 14.6 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
target,2461243.6814,11.85,0.05,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 20260722.1814 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.92 23:33:37.46 +53:41:37.4
111.46127 -7.43606 galactic Cas Second-epoch detections are separated by 1.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:33:37.46 +53:41:37.4 (user input) | T | P | (position from user input) J-Ks=0.654+/-0.047 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:37.46 +53:41:37.4: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:37.46 +53:41:37.4: 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 22.1814* 23 33 37.46 +53 41 37.4 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,2461243.6814,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260722.1814 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.54 00:20:11.75 +53:51:53.3
118.28151 -8.72461 galactic Cas Second-epoch detections are separated by 4.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:20:11.75 +53:51:53.3 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:11.75 +53:51:53.3: 12.72 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:11.75 +53:51:53.3: 12.64 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 00 20 11.75 +53 51 53.3 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
target,2461243.6814,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260722.1814 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.62 00:03:07.81 +50:05:54.2
115.04453 -12.03210 galactic Cas Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 393901002723435648 | 00:03:08.33 +50:06:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.795+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:07.81 +50:05:54.2: 13.03 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:07.81 +50:05:54.2: 13.21 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 00 03 07.81 +50 05 54.2 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 393901002723435648,2461243.6814,11.62,0.05,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
Gaia DR3 393901002723435648 20260722.1814 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 22.1814 2461243.6814 11.89 23:23:22.55 +53:36:20.0
109.98156 -7.03734 galactic Cas Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1995798429747316736 | 23:23:25.49 +53:36:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.178+/-0.036 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:22.55 +53:36:20.0: 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 23:23:22.55 +53:36:20.0: 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 22.1814* 23 23 22.55 +53 36 20.0 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 1995798429747316736,2461243.6814,11.89,0.05,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
Gaia DR3 1995798429747316736 20260722.1814 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 22.1814 2461243.6814 11.63 00:00:37.81 +56:39:40.2
115.95864 -5.52112 galactic Cas Second-epoch detections are separated by 0.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J000.1534+56.6624 | 00:00:36.83 +56:39:20.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=1.169+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:37.81 +56:39:40.2: 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 00:00:37.81 +56:39:40.2: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 00 00 37.81 +56 39 40.2 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
ATO J000.1534+56.6624,2461243.6814,11.63,0.05,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 J000.1534+56.6624 20260722.1814 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 22.1814 2461243.6814 11.69 23:18:18.62 +56:19:03.0
110.23424 -4.24103 galactic Cas Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 23:18:18.62 +56:19:03.0: 13.38 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:18.62 +56:19:03.0: 13.29 +/- 0.29 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 18 18.62 +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+56.3050,2461243.6814,11.69,0.05,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
ATO J349.5618+56.3050 20260722.1814 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 22.1814 2461243.6814 11.48 23:54:46.56 +55:01:23.6
114.80737 -6.95222 galactic Cas Second-epoch detections are separated by 0.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993908884658311424 | 23:54:48.46 +55:01:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.509+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:46.56 +55:01:23.6: 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 23:54:46.56 +55:01:23.6: 13.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 54 46.56 +55 01 23.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993908884658311424,2461243.6814,11.48,0.05,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 1993908884658311424 20260722.1814 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 22.1814 2461243.6814 11.69 23:19:10.07 +50:19:12.1
108.22034 -9.89745 galactic And Second-epoch detections are separated by 3.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1990867665553782784 | 23:19:09.04 +50:19:43.8 (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 23:19:10.07 +50:19:12.1: 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 23:19:10.07 +50:19:12.1: 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 22.1814* 23 19 10.07 +50 19 12.1 11.7 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 1990867665553782784,2461243.6814,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1990867665553782784 20260722.1814 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 22.1814 2461243.6814 11.45 23:57:47.11 +56:40:12.2
115.57589 -5.43346 galactic Cas Second-epoch detections are separated by 3.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J359.4451+56.6691 | 23:57:43.94 +56:39:42.8 (Gaia DR3) | DBH (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 23:57:47.11 +56:40:12.2: 12.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:47.11 +56:40:12.2: 12.68 +/- 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 22.1814* 23 57 47.11 +56 40 12.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.4451+56.6691,2461243.6814,11.45,0.05,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 J359.4451+56.6691 20260722.1814 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 22.1814 2461243.6814 11.73 23:19:10.58 +56:55:23.4
110.55919 -3.71574 galactic Cas Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:19:10.58 +56:55:23.4 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:10.58 +56:55:23.4: 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 23:19:10.58 +56:55:23.4: 13.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 19 10.58 +56 55 23.4 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,2461243.6814,11.73,0.05,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
target 20260722.1814 11.73CV 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 22.1814 2461243.6814 11.64 23:12:47.09 +54:51:26.3
108.97255 -5.31835 galactic Cas Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.1994+54.8570 | 23:12:47.09 +54:51:26.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=1.007+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:47.09 +54:51:26.3: 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 23:12:47.09 +54:51:26.3: 13.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 12 47.09 +54 51 26.3 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
ATO J348.1994+54.8570,2461243.6814,11.64,0.05,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
ATO J348.1994+54.8570 20260722.1814 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 22.1814 2461243.6814 11.57 23:12:15.21 +56:31:11.3
109.52578 -3.74820 galactic Cas Second-epoch detections are separated by 0.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:12:15.21 +56:31:11.3 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:15.21 +56:31:11.3: 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 23:12:15.21 +56:31:11.3: 13.27 +/- 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 22.1814* 23 12 15.21 +56 31 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,2461243.6814,11.57,0.05,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 20260722.1814 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 22.1814 2461243.6814 11.36 00:19:06.08 +56:05:28.6
118.40319 -6.49587 galactic Cas Second-epoch detections are separated by 2.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.7658+56.1014 | 00:19:06.08 +56:05:28.6 (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 00:19:06.08 +56:05:28.6: 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 00:19:06.08 +56:05:28.6: 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 22.1814* 00 19 06.08 +56 05 28.6 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J004.7658+56.1014,2461243.6814,11.36,0.05,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
ATO J004.7658+56.1014 20260722.1814 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 22.1814 2461243.6814 11.46 23:35:27.57 +55:35:10.2
112.27861 -5.70616 galactic Cas Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1997479239433053696 | 23:35:24.49 +55:35:06.4 (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 23:35:27.57 +55:35:10.2: 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 23:35:27.57 +55:35:10.2: 13.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 35 27.57 +55 35 10.2 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997479239433053696,2461243.6814,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997479239433053696 20260722.1814 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.21 00:14:56.88 +55:03:50.8
117.67842 -7.43500 galactic Cas Second-epoch detections are separated by 0.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 420570108229652736 | 00:14:56.88 +55:03:50.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G5 (LAMOST DR5) J-Ks=0.770+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:56.88 +55:03:50.8: 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 00:14:56.88 +55:03:50.8: 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 22.1814* 00 14 56.88 +55 03 50.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 420570108229652736,2461243.6814,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 420570108229652736 20260722.1814 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.23 00:07:20.94 +55:34:40.6
116.68388 -6.75804 galactic Cas Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:07:20.94 +55:34:40.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.514+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:20.94 +55:34:40.6: 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 00:07:20.94 +55:34:40.6: 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 22.1814* 00 07 20.94 +55 34 40.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461243.6814,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260722.1814 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.39 23:41:40.67 +53:02:02.0
112.43481 -8.41017 galactic Cas Second-epoch detections are separated by 1.6" and 6.3 pix
The object was found in VSX 6" Gaia DR3 1993084388375081088
Type: ROT
# Max. Min./Amp. JD0 Period
15.200 G 15.230 G G
ATTENTION: measured mag 11.39 is 3.8 mag brighter than the VSX record maximum brightness 15.20 - 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 23:41:40.67 +53:02:02.0: 12.57 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:40.67 +53:02:02.0: 12.27 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 41 40.67 +53 02 02.0 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 1993084388375081088,2461243.6814,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993084388375081088 20260722.1814 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.52 23:28:57.55 +51:01:10.4
109.94177 -9.76007 galactic Cas Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:57.55 +51:01:10.4 (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 23:28:57.55 +51:01:10.4: 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 23:28:57.55 +51:01:10.4: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 28 57.55 +51 01 10.4 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
target,2461243.6814,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260722.1814 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.52 23:14:10.71 +54:09:43.9
108.90237 -6.03892 galactic Cas Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.5351+54.1603 | 23:14:08.43 +54:09:37.1 (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 23:14:10.71 +54:09:43.9: 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 23:14:10.71 +54:09:43.9: 13.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 14 10.71 +54 09 43.9 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 J348.5351+54.1603,2461243.6814,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.5351+54.1603 20260722.1814 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.54 23:18:16.20 +51:58:43.0
108.68298 -8.29681 galactic And Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J349.5709+51.9791 | 23:18:16.20 +51:58:43.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.262+/-0.035 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:16.20 +51:58:43.0: 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 23:18:16.20 +51:58:43.0: 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 22.1814* 23 18 16.20 +51 58 43.0 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
ATO J349.5709+51.9791,2461243.6814,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.5709+51.9791 20260722.1814 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 10.95 00:30:31.21 +55:56:24.7
119.98510 -6.81182 galactic Cas Second-epoch detections are separated by 1.4" and 5.7 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 10.95 is 3.7 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 00:30:31.21 +55:56:24.7: 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 00:30:31.21 +55:56:24.7: 13.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 00 30 31.21 +55 56 24.7 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 421275548023447040,2461243.6814,10.95,0.05,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
Gaia DR3 421275548023447040 20260722.1814 10.95CV 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 22.1814 2461243.6814 11.23 23:49:49.43 +54:19:20.5
113.94323 -7.47055 galactic Cas Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J357.4334+54.3270 | 23:49:48.43 +54:19:45.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.775+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:49.43 +54:19:20.5: 13.63 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:49.43 +54:19:20.5: 13.51 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.63 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 49 49.43 +54 19 20.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.4334+54.3270,2461243.6814,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.4334+54.3270 20260722.1814 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 10.72 23:46:36.44 +51:42:14.8
112.81916 -9.89016 galactic Cas Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 23:46:36.44 +51:42:14.8: 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 23:46:36.44 +51:42:14.8: 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 22.1814* 23 46 36.44 +51 42 14.8 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 1945016110828646912,2461243.6814,10.72,0.05,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 1945016110828646912 20260722.1814 10.72CV 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 22.1814 2461243.6814 10.84 23:21:14.36 +55:23:13.6
110.29631 -5.25628 galactic Cas Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996852414723764608 | 23:21:11.12 +55:23:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5) J-Ks=0.546+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:14.36 +55:23:13.6: 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 23:21:14.36 +55:23:13.6: 13.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 21 14.36 +55 23 13.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996852414723764608,2461243.6814,10.84,0.05,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 1996852414723764608 20260722.1814 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 10.02 23:36:32.76 +50:40:33.6
110.99429 -10.45171 galactic And Second-epoch detections are separated by 2.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1944540365891633792 | 23:36:31.17 +50:40:21.7 (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 23:36:32.76 +50:40:33.6: 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 23:36:32.76 +50:40:33.6: 13.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 36 32.76 +50 40 33.6 10.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944540365891633792,2461243.6814,10.02,0.05,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 1944540365891633792 20260722.1814 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 10.00 23:50:25.79 +49:51:13.8
112.95272 -11.83213 galactic Cas Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1940880469640450304 | 23:50:26.96 +49:51:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.045+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:25.79 +49:51:13.8: 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 23:50:25.79 +49:51:13.8: 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 22.1814* 23 50 25.79 +49 51 13.8 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940880469640450304,2461243.6814,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940880469640450304 20260722.1814 10.00CV 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 22.1814 2461243.6814 10.12 23:27:26.44 +49:36:03.6
109.24473 -11.02539 galactic And Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was found in ASASSN-V 3" ASASSN-V J232726.19+493602.3
Type: L
MeanMag 11.8 m Amp. 0.09 m Period d
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 23:27:26.44 +49:36:03.6: 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 23:27:26.44 +49:36:03.6: 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 22.1814* 23 27 26.44 +49 36 03.6 10.1 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
VARIABLE_NAME,2461243.6814,10.12,0.05,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
VARIABLE_NAME 20260722.1814 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 9.61 00:15:19.60 +53:12:02.7
117.46667 -9.28737 galactic Cas Second-epoch detections are separated by 0.8" and 6.1 pix
The object was found in VSX 2" 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 00:15:19.60 +53:12:02.7: 13.24 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:19.60 +53:12:02.7: 13.15 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 22.1814* 00 15 19.60 +53 12 02.7 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419244578251557888,2461243.6814,9.61,0.05,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
Gaia DR3 419244578251557888 20260722.1814 9.61CV 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 22.1814 2461243.6814 10.37 00:03:30.72 +53:19:18.5
115.72203 -8.87771 galactic Cas Second-epoch detections are separated by 0.5" and 6.3 pix
The object was found in VSX 2" Gaia DR3 396248700568406016
Type: ROT
# Max. Min./Amp. JD0 Period
12.400 G 12.440 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 00:03:30.72 +53:19:18.5: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:30.72 +53:19:18.5: 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 22.1814* 00 03 30.72 +53 19 18.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 396248700568406016,2461243.6814,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 396248700568406016 20260722.1814 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.02 23:23:03.72 +55:52:05.9
110.70318 -4.89094 galactic Cas Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.7593+55.8722 | 23:23:05.90 +55:52:41.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9 1928AnHar.100...49C HD 240277 J-Ks=0.843+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:03.72 +55:52:05.9: 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 23:23:03.72 +55:52:05.9: 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 22.1814* 23 23 03.72 +55 52 05.9 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
ATO J350.7593+55.8722,2461243.6814,11.02,0.05,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
ATO J350.7593+55.8722 20260722.1814 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 22.1814 2461243.6814 10.90 23:29:11.99 +53:11:19.5
110.67227 -7.71422 galactic Cas Second-epoch detections are separated by 2.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1992540782954086144 | 23:29:14.93 +53:11:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:11.99 +53:11:19.5: 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 23:29:11.99 +53:11:19.5: 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 22.1814* 23 29 11.99 +53 11 19.5 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 1992540782954086144,2461243.6814,10.90,0.05,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 1992540782954086144 20260722.1814 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.03 23:59:13.16 +53:28:26.4
115.11713 -8.60357 galactic Cas Second-epoch detections are separated by 0.6" and 6.1 pix
The object was found in VSX 0" Gaia DR3 1945272778076258944
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.320 G 13.360 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 23:59:13.16 +53:28:26.4: 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 23:59:13.16 +53:28:26.4: 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 22.1814* 23 59 13.16 +53 28 26.4 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1945272778076258944,2461243.6814,11.03,0.05,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
Gaia DR3 1945272778076258944 20260722.1814 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 22.1814 2461243.6814 11.27 23:25:04.90 +55:05:34.6
110.71525 -5.71732 galactic Cas Second-epoch detections are separated by 1.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:04.90 +55:05:34.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.363+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:04.90 +55:05:34.6: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:04.90 +55:05:34.6: 13.29 +/- 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 22.1814* 23 25 04.90 +55 05 34.6 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
target,2461243.6814,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260722.1814 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.56 23:21:39.15 +55:10:51.5
110.28101 -5.47010 galactic Cas Second-epoch detections are separated by 1.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996925326080484992 | 23:21:41.10 +55:10:09.2 (Gaia DR3) | RS (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:39.15 +55:10:51.5: 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 23:21:39.15 +55:10:51.5: 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 22.1814* 23 21 39.15 +55 10 51.5 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 1996925326080484992,2461243.6814,11.56,0.05,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 1996925326080484992 20260722.1814 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 22.1814 2461243.6814 11.34 23:57:13.73 +56:42:29.5
115.50884 -5.38024 galactic Cas Second-epoch detections are separated by 4.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J359.2913+56.7049 | 23:57:10.40 +56:42:49.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K4III 1958ApJ...128..174B NGC 7789 494 J-Ks=0.424+/-0.110 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:13.73 +56:42:29.5: 12.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:13.73 +56:42:29.5: 12.23 +/- 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 22.1814* 23 57 13.73 +56 42 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 J359.2913+56.7049,2461243.6814,11.34,0.05,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 J359.2913+56.7049 20260722.1814 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.31 23:56:52.56 +52:09:35.1
114.48917 -9.81532 galactic Cas Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:56:52.56 +52:09:35.1 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:52.56 +52:09:35.1: 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 23:56:52.56 +52:09:35.1: 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 22.1814* 23 56 52.56 +52 09 35.1 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461243.6814,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260722.1814 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.48 23:34:32.76 +49:44:28.9
110.40254 -11.25058 galactic And Second-epoch detections are separated by 1.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.6511+49.7393 | 23:34:32.76 +49:44:28.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:32.76 +49:44:28.9: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:32.76 +49:44:28.9: 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 22.1814* 23 34 32.76 +49 44 28.9 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
ATO J353.6511+49.7393,2461243.6814,11.48,0.05,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
ATO J353.6511+49.7393 20260722.1814 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 22.1814 2461243.6814 11.57 23:19:31.93 +55:36:24.0
110.14476 -4.96668 galactic Cas Second-epoch detections are separated by 3.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996916972372159360 | 23:19:35.92 +55:36:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.852+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:31.93 +55:36:24.0: 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 23:19:31.93 +55:36:24.0: 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 22.1814* 23 19 31.93 +55 36 24.0 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
Gaia DR3 1996916972372159360,2461243.6814,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996916972372159360 20260722.1814 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 22.1814 2461243.6814 11.57 23:41:49.92 +54:40:26.7
112.90179 -6.83647 galactic Cas Second-epoch detections are separated by 1.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.4769+54.6722 | 23:41:49.92 +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 23:41:49.92 +54:40:26.7: 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 23:41:49.92 +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 22.1814* 23 41 49.92 +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+54.6722,2461243.6814,11.57,0.05,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 J355.4769+54.6722 20260722.1814 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 22.1814 2461243.6814 11.70 23:12:17.78 +57:05:09.1
109.74325 -3.22538 galactic Cas Second-epoch detections are separated by 2.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.0943+57.0885 | 23:12:22.53 +57:04:44.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M4II 2018MNRAS.475.2003D IRAS 23101+5648
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:17.78 +57:05:09.1: 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 23:12:17.78 +57:05:09.1: 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 22.1814* 23 12 17.78 +57 05 09.1 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
ATO J348.0943+57.0885,2461243.6814,11.70,0.05,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 20260722.1814 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.69 23:34:08.29 +54:02:57.0
111.64089 -7.11931 galactic Cas Second-epoch detections are separated by 1.3" and 6.2 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 +54:02:57.0: 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 23:34:08.29 +54:02:57.0: 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 22.1814* 23 34 08.29 +54 02 57.0 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 1994286807419596416,2461243.6814,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994286807419596416 20260722.1814 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 22.1814 2461243.6814 11.72 23:29:23.95 +51:39:58.1
110.21559 -9.16860 galactic Cas Second-epoch detections are separated by 1.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1991424538127002368 | 23:29:23.95 +51:39:58.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.374+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:23.95 +51:39:58.1: 13.28 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:23.95 +51:39:58.1: 13.12 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 22.1814* 23 29 23.95 +51 39 58.1 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
Large-amplitude variable Gaia DR2 1991424538127002368,2461243.6814,11.72,0.05,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
Large-amplitude variable Gaia DR2 1991424538127002368 20260722.1814 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 22.1814 2461243.6814 11.72 23:25:28.09 +49:20:11.4
108.84772 -11.16988 galactic And Second-epoch detections are separated by 2.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:28.09 +49:20:11.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:28.09 +49:20:11.4: 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 23:25:28.09 +49:20:11.4: 13.55 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 23 25 28.09 +49 20 11.4 11.7 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,2461243.6814,11.72,0.05,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 20260722.1814 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 22.1814 2461243.6814 11.60 00:06:05.70 +53:15:52.3
116.09567 -9.00430 galactic Cas Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 396192281879188224 | 00:06:08.02 +53:16:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.400+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:05.70 +53:15:52.3: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:05.70 +53:15:52.3: 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 22.1814* 00 06 05.70 +53 15 52.3 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
Gaia DR3 396192281879188224,2461243.6814,11.60,0.05,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 396192281879188224 20260722.1814 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.93 23:28:27.39 +53:49:28.8
110.76953 -7.07602 galactic Cas Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 23:28:27.39 +53:49:28.8: 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 23:28:27.39 +53:49:28.8: 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 22.1814* 23 28 27.39 +53 49 28.8 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+53.8121,2461243.6814,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.1131+53.8121 20260722.1814 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.74 00:04:53.66 +51:59:43.1
115.68250 -10.22010 galactic Cas Second-epoch detections are separated by 2.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.2174+52.0011 | 00:04:53.66 +51:59:43.1 (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 00:04:53.66 +51:59:43.1: 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 00:04:53.66 +51:59:43.1: 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 22.1814* 00 04 53.66 +51 59 43.1 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
ATO J001.2174+52.0011,2461243.6814,11.74,0.05,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
ATO J001.2174+52.0011 20260722.1814 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 22.1814 2461243.6814 11.75 23:42:14.39 +51:45:07.7
112.16924 -9.66773 galactic Cas Second-epoch detections are separated by 1.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:42:14.39 +51:45:07.7 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:14.39 +51:45:07.7: 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 23:42:14.39 +51:45:07.7: 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 22.1814* 23 42 14.39 +51 45 07.7 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,2461243.6814,11.75,0.05,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 20260722.1814 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 22.1814 2461243.6814 11.89 00:18:38.34 +56:24:55.5
118.38047 -6.16621 galactic Cas Second-epoch detections are separated by 0.4" and 5.9 pix
The object was found in VSX11" Gaia DR3 421583789236879744
Type: ROT
# Max. Min./Amp. JD0 Period
15.380 G 15.420 G G
ATTENTION: measured mag 11.89 is 3.5 mag brighter than the VSX record maximum brightness 15.38 - 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 00:18:38.34 +56:24:55.5: 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 00:18:38.34 +56:24:55.5: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 22.1814* 00 18 38.34 +56 24 55.5 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
Gaia DR3 421583789236879744,2461243.6814,11.89,0.05,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
Gaia DR3 421583789236879744 20260722.1814 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 22.1814 2461243.6814 12.62 23:16:28.71 +51:57:40.0
108.41639 -8.21413 galactic And Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:16:28.71 +51:57:40.0 (user input) | T | P | (position from user input) J-Ks=0.531+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:28.71 +51:57:40.0: 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 23:16:28.71 +51:57:40.0: 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 22.1814* 23 16 28.71 +51 57 40.0 12.6 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,2461243.6814,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260722.1814 12.62CV 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 22.1814 2461243.6814 11.67 23:26:01.28 +49:55:46.3
109.13373 -10.63994 galactic And Second-epoch detections are separated by 2.5" and 6.1 pix
The object was found in VSX 3" 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 23:26:01.28 +49:55:46.3: 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 23:26:01.28 +49:55:46.3: 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 22.1814* 23 26 01.28 +49 55 46.3 11.7 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 1943087155117309568,2461243.6814,11.67,0.05,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
Gaia DR3 1943087155117309568 20260722.1814 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 22.1814 2461243.6814 10.63 23:21:11.95 +50:00:12.0
108.41707 -10.30808 galactic And Second-epoch detections are separated by 1.3" and 6.4 pix
The object was found in VSX 3" 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 23:21:11.95 +50:00:12.0: 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 23:21:11.95 +50:00:12.0: 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 22.1814* 23 21 11.95 +50 00 12.0 10.6 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
AK And,2461243.6814,10.63,0.05,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
AK And 20260722.1814 10.63CV 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
## 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: 2461243.68181705 22.07.2026 04:21:38.993 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
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: 19 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): 21546
Objects passed selection criteria: 21493
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 17686.5
Average stars matched: 16756.2 (94.7403 %)
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 Tue Jul 21 15:05:04 CDT 2026
VaST build number 1.0rc89-162-g0b3e9b13
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 22 00:16:59 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: 2461243.68181705 22.07.2026 04:21:38.993 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 250
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: 138 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): 161688
Objects passed selection criteria: 161316
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 141546
Average stars matched: 134902 (95.3056 %)
Memory usage VmPeak: 1998076 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 21 15:05:04 CDT 2026
VaST build number 1.0rc89-162-g0b3e9b13
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 22 00:25:13 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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: 2461243.68098924
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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
Image size: 938.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:02.052 +53:59:43.86 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 00:00:02.052 +53:59:43.86
Angular distance between the image centers 0.0257 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Image size: 938.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:05.694 +53:59:26.82 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 00:00:05.694 +53:59:26.82
Angular distance between the image centers 0.0343 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 00:00:02.052 +53:59:43.86
Second-epoch second image center 00:00:05.694 +53:59:26.82
Angular distance between the image centers 0.01010 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.S5L9DXWBwL
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.9qrd2PopAn
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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits &> /tmp/tmp.slQpPj0T3x
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits &> /tmp/tmp.OhgsB73A8k
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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 4 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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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
14.2 mag. fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
14.2 mag. fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.3 (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.S5L9DXWBwL (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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/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.9qrd2PopAn (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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/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.slQpPj0T3x (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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.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=1082, bad_region=2871, passed=14802
Got 14802 stars (including 10998 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat
util/solve_plate_with_UCAC5 got 14802 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8500 through 0 to 14.6558, gap 14.6558 to 344.8500
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 344.8487 through 0 to 14.6562, gap 14.6562 to 344.8487
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits N_match=972 sigma_overall_arcsec=0.609 sigma_q1_arcsec=0.627 sigma_q2_arcsec=0.647 sigma_q3_arcsec=0.597 sigma_q4_arcsec=0.568 n_q1=316 n_q2=191 n_q3=274 n_q4=191 worst_quadrant_to_overall_ratio=1.063
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.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.OhgsB73A8k (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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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=1098, bad_region=2861, passed=14913
Got 14913 stars (including 11103 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat
util/solve_plate_with_UCAC5 got 14913 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8500 through 0 to 14.8382, gap 14.8382 to 344.8500
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 12422 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8486 through 0 to 14.8384, gap 14.8384 to 344.8486
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 12422 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 12422 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits N_match=970 sigma_overall_arcsec=0.579 sigma_q1_arcsec=0.543 sigma_q2_arcsec=0.640 sigma_q3_arcsec=0.613 sigma_q4_arcsec=0.586 n_q1=313 n_q2=191 n_q3=274 n_q4=192 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits sigma_overall=0.609 worst_q_ratio=1.063
new2=fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits sigma_overall=0.579 worst_q_ratio=1.104
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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110_astrometric_residuals.png (972 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111_astrometric_residuals.png (970 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:08:53.76 +54:52:27.2: 15.40 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:53.76 +54:52:27.2: 15.74 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.40 +/- 0.31
Forced photometry filter KEPT candidate at 00:08:53.76 +54:52:27.2: ref_mag=15.40 +/- 0.31 new_mean_mag=11.3916 delta=4.01 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out33554.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33554_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 33554_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:08:53.76 +54:52:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 1.090 420235238226090240 002.22353179966 +54.87436037821 11.3734 11.0781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21482_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 21482_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:44:31.90 +56:34:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06239_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 06239_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:58:25.13 +51:23:24.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07077_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 07077_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:09:36.51 +51:34:00.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
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 --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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
Image size: 938.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:02.052 +53:59:43.86 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 00:00:02.052 +53:59:43.86
Angular distance between the image centers 0.0257 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Image size: 938.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:05.694 +53:59:26.82 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 00:00:05.694 +53:59:26.82
Angular distance between the image centers 0.0343 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 00:00:02.052 +53:59:43.86
Second-epoch second image center 00:00:05.694 +53:59:26.82
Angular distance between the image centers 0.01010 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.m1m4AQhKjw
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.1BGAWD5aC7
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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits &> /tmp/tmp.ctvyuIDGvt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits &> /tmp/tmp.A4JfjIyGeA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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 198 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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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
12.5 mag. fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
12.5 mag. fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 11.9 (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.m1m4AQhKjw (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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/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.1BGAWD5aC7 (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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/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.ctvyuIDGvt (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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.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=29, blended=11124, bad_region=15456, passed=123645
Got 123645 stars (including 98212 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat
util/solve_plate_with_UCAC5 got 123645 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8500 through 0 to 14.8253, gap 14.8253 to 344.8500
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 110524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8488 through 0 to 14.8257, gap 14.8257 to 344.8488
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 110525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 110525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits N_match=973 sigma_overall_arcsec=0.571 sigma_q1_arcsec=0.619 sigma_q2_arcsec=0.570 sigma_q3_arcsec=0.575 sigma_q4_arcsec=0.541 n_q1=314 n_q2=190 n_q3=269 n_q4=200 worst_quadrant_to_overall_ratio=1.084
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.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.A4JfjIyGeA (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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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=22, blended=11162, bad_region=15518, passed=122674
Got 122674 stars (including 97163 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat
util/solve_plate_with_UCAC5 got 122674 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8500 through 0 to 14.8381, gap 14.8381 to 344.8500
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 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: 974 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 109647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8486 through 0 to 14.8384, gap 14.8384 to 344.8486
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 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: 974 matched stars entering correct_measured_positions(), 109647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 109646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits N_match=974 sigma_overall_arcsec=0.563 sigma_q1_arcsec=0.595 sigma_q2_arcsec=0.572 sigma_q3_arcsec=0.584 sigma_q4_arcsec=0.606 n_q1=309 n_q2=192 n_q3=275 n_q4=198 worst_quadrant_to_overall_ratio=1.076
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-20-27_20.00sec_5.00C_LIGHT_0110.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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_2026-07-22_CI_Cas-04-Q2b1x1_000713_TTUQ2b1x1_1648398_NGUWJaRy/wcs_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:16.50 +51:27:00.4: 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 23:43:58.89 +55:38:49.6: 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 23:41:11.48 +57:06:44.9: 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 00:01:47.63 +56:08:37.0: 13.63 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:21.72 +53:48:15.8: 13.00 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:54.31 +51:24:50.5: 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 23:23:45.48 +55:35:38.4: 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 23:43:36.04 +52:28:00.5: 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 00:04:07.71 +56:06:31.4: 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 00:01:47.63 +56:08:37.0: 13.17 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:58.89 +55:38:49.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:11.48 +57:06:44.9: 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 00:12:16.50 +51:27:00.4: 13.63 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.34 +/- 0.18
Forced photometry filter KEPT candidate at 00:01:47.63 +56:08:37.0: ref_mag=13.34 +/- 0.18 new_mean_mag=12.0267 delta=1.31 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:53:54.31 +51:24:50.5: 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 23:39:21.72 +53:48:15.8: 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 23:43:36.04 +52:28:00.5: 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 23:23:45.48 +55:35:38.4: 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 00:04:07.71 +56:06:31.4: 13.56 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.96 +/- 0.12
Forced photometry filter REJECTED candidate at 23:39:21.72 +53:48:15.8: ref_mag=12.96 +/- 0.12 new_mean_mag=12.2768 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 00:07:14.46 +56:13:57.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:14.46 +56:13:57.1: 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 23:36:17.09 +55:23:41.9: 12.46 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:17.09 +55:23:41.9: 12.23 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.08
Forced photometry filter REJECTED candidate at 23:36:17.09 +55:23:41.9: ref_mag=12.34 +/- 0.08 new_mean_mag=12.1162 delta=0.22 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:15.08 +52:45:11.3: 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 23:46:15.08 +52:45:11.3: 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 23:40:15.74 +52:16:46.3: 13.59 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:40:15.74 +52:16:46.3: 13.29 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.18
Forced photometry filter KEPT candidate at 23:40:15.74 +52:16:46.3: ref_mag=13.42 +/- 0.18 new_mean_mag=11.9907 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 23:45:47.77 +57:16:14.9: 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 23:45:47.77 +57:16:14.9: 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 23:31:48.19 +56:54:17.7: 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 23:37:08.58 +50:09:11.0: 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 23:31:48.19 +56:54:17.7: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:34.18 +53:02:54.6: 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 23:37:08.58 +50:09:11.0: 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 23:47:35.26 +55:28:20.1: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:31.92 +55:18:14.6: 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 23:44:34.18 +53:02:54.6: 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 23:47:35.26 +55:28:20.1: 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 23:39:31.92 +55:18:14.6: 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 23:33:37.46 +53:41:37.4: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:11.75 +53:51:53.3: 12.72 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:37.46 +53:41:37.4: 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 00:20:11.75 +53:51:53.3: 12.64 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.11
Forced photometry filter KEPT candidate at 00:20:11.75 +53:51:53.3: ref_mag=12.69 +/- 0.11 new_mean_mag=11.4743 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:07.81 +50:05:54.2: 13.03 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:07.81 +50:05:54.2: 13.21 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.13
Forced photometry filter KEPT candidate at 00:03:07.81 +50:05:54.2: ref_mag=13.10 +/- 0.13 new_mean_mag=11.6054 delta=1.49 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:14.12 +55:25:05.5: 12.67 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:22.55 +53:36:20.0: 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 23:54:14.12 +55:25:05.5: 12.43 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.10
Forced photometry filter REJECTED candidate at 23:54:14.12 +55:25:05.5: ref_mag=12.54 +/- 0.10 new_mean_mag=11.8775 delta=0.66 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:22.55 +53:36:20.0: 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 23:52:57.96 +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 23:52:57.96 +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 23:52:57.96 +56:09:30.6: ref_mag=11.68 +/- 0.04 new_mean_mag=11.7628 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:37.81 +56:39:40.2: 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 00:00:37.81 +56:39:40.2: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:40.63 +56:24:48.4: 12.06 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:40.63 +56:24:48.4: 11.83 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.05
Forced photometry filter REJECTED candidate at 23:56:40.63 +56:24:48.4: ref_mag=11.94 +/- 0.05 new_mean_mag=11.5310 delta=0.41 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:33.94 +56:38:56.2: 11.84 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:33.94 +56:38:56.2: 11.38 +/- 0.12 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.09
Forced photometry filter REJECTED candidate at 23:57:33.94 +56:38:56.2: ref_mag=11.56 +/- 0.09 new_mean_mag=11.5699 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:18.62 +56:19:03.0: 13.38 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:18.62 +56:19:03.0: 13.29 +/- 0.29 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.20
Forced photometry filter KEPT candidate at 23:18:18.62 +56:19:03.0: ref_mag=13.34 +/- 0.20 new_mean_mag=11.6763 delta=1.66 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:30.95 +52:04:53.6: 12.76 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:30.95 +52:04:53.6: 12.38 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.09
Forced photometry filter REJECTED candidate at 23:22:30.95 +52:04:53.6: ref_mag=12.53 +/- 0.09 new_mean_mag=11.6374 delta=0.89 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:46.56 +55:01:23.6: 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 23:19:10.07 +50:19:12.1: 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 23:54:46.56 +55:01:23.6: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:10.07 +50:19:12.1: 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 23:57:47.11 +56:40:12.2: 12.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:10.58 +56:55:23.4: 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 23:57:47.11 +56:40:12.2: 12.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:10.58 +56:55:23.4: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:47.09 +54:51:26.3: 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 23:12:15.21 +56:31:11.3: 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 23:12:47.09 +54:51:26.3: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:15.21 +56:31:11.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:06.08 +56:05:28.6: 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 00:19:06.08 +56:05:28.6: 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 23:35:27.57 +55:35:10.2: 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 23:35:27.57 +55:35:10.2: 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 00:14:56.88 +55:03:50.8: 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 00:14:56.88 +55:03:50.8: 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 00:07:20.94 +55:34:40.6: 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 00:07:20.94 +55:34:40.6: 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 23:41:40.67 +53:02:02.0: 12.57 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:40.67 +53:02:02.0: 12.27 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.07
Forced photometry filter KEPT candidate at 23:41:40.67 +53:02:02.0: ref_mag=12.39 +/- 0.07 new_mean_mag=11.3883 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:28.16 +56:13:38.2: 10.54 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:28.16 +56:13:38.2: 10.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.01
Forced photometry filter REJECTED candidate at 23:56:28.16 +56:13:38.2: ref_mag=10.38 +/- 0.01 new_mean_mag=11.2728 delta=-0.90 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:57.55 +51:01:10.4: 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 23:14:10.71 +54:09:43.9: 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 23:28:57.55 +51:01:10.4: 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 23:14:10.71 +54:09:43.9: 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 00:30:31.21 +55:56:24.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:16.20 +51:58:43.0: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:49.43 +54:19:20.5: 13.63 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:31.21 +55:56:24.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:16.20 +51:58:43.0: 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 23:49:49.43 +54:19:20.5: 13.51 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.63 +/- 0.35
Forced photometry filter KEPT candidate at 23:49:49.43 +54:19:20.5: ref_mag=13.63 +/- 0.35 new_mean_mag=11.2347 delta=2.39 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:36.44 +51:42:14.8: 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 23:46:36.44 +51:42:14.8: 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 23:21:14.36 +55:23:13.6: 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 23:21:14.36 +55:23:13.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:32.76 +50:40:33.6: 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 23:36:32.76 +50:40:33.6: 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 23:50:25.79 +49:51:13.8: 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 23:27:26.44 +49:36:03.6: 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 23:50:25.79 +49:51:13.8: 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 23:27:26.44 +49:36:03.6: 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 00:15:19.60 +53:12:02.7: 13.24 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:19.60 +53:12:02.7: 13.15 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.16
Forced photometry filter KEPT candidate at 00:15:19.60 +53:12:02.7: ref_mag=13.20 +/- 0.16 new_mean_mag=9.5881 delta=3.61 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:30.72 +53:19:18.5: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:30.72 +53:19:18.5: 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 23:23:03.72 +55:52:05.9: 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 23:23:03.72 +55:52:05.9: 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 23:57:55.60 +56:28:28.3: 10.76 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:11.99 +53:11:19.5: 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 23:57:55.60 +56:28:28.3: 10.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.60 +/- 0.03
Forced photometry filter REJECTED candidate at 23:57:55.60 +56:28:28.3: ref_mag=10.60 +/- 0.03 new_mean_mag=10.9402 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:11.99 +53:11:19.5: 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 23:59:13.16 +53:28:26.4: 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 23:59:13.16 +53:28:26.4: 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 23:25:04.90 +55:05:34.6: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:04.90 +55:05:34.6: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:56.50 +53:10:41.3: 9.67 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:56.50 +53:10:41.3: 9.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.41 +/- 0.01
Forced photometry filter REJECTED candidate at 23:17:56.50 +53:10:41.3: ref_mag=9.41 +/- 0.01 new_mean_mag=11.4808 delta=-2.07 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:39.15 +55:10:51.5: 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 23:57:13.73 +56:42:29.5: 12.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:39.15 +55:10:51.5: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:13.73 +56:42:29.5: 12.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:52.56 +52:09:35.1: 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 23:56:52.56 +52:09:35.1: 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 23:28:13.80 +57:49:26.8: 11.92 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:13.80 +57:49:26.8: 11.72 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.05
Forced photometry filter REJECTED candidate at 23:28:13.80 +57:49:26.8: ref_mag=11.82 +/- 0.05 new_mean_mag=11.5801 delta=0.23 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:32.76 +49:44:28.9: 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 23:19:31.93 +55:36:24.0: 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 23:34:32.76 +49:44:28.9: 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 23:19:31.93 +55:36:24.0: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:49.92 +54:40:26.7: 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 23:41:49.92 +54:40:26.7: 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 23:12:17.78 +57:05:09.1: 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 23:12:17.78 +57:05:09.1: 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 23:57:53.62 +56:29:19.5: 11.12 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:53.62 +56:29:19.5: 10.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.04
Forced photometry filter REJECTED candidate at 23:57:53.62 +56:29:19.5: ref_mag=10.96 +/- 0.04 new_mean_mag=11.5128 delta=-0.55 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.29 +54:02:57.0: 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 23:34:08.29 +54:02:57.0: 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 00:12:35.76 +57:14:05.7: 10.85 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:12.73 +54:21:35.6: 11.92 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:23.95 +51:39:58.1: 13.28 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:35.76 +57:14:05.7: 10.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.03
Forced photometry filter REJECTED candidate at 00:12:35.76 +57:14:05.7: ref_mag=10.78 +/- 0.03 new_mean_mag=11.5296 delta=-0.75 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:12.73 +54:21:35.6: 11.77 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.05
Forced photometry filter REJECTED candidate at 23:52:12.73 +54:21:35.6: ref_mag=11.84 +/- 0.05 new_mean_mag=11.6710 delta=0.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:23.95 +51:39:58.1: 13.12 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.16
Forced photometry filter KEPT candidate at 23:29:23.95 +51:39:58.1: ref_mag=13.20 +/- 0.16 new_mean_mag=11.7247 delta=1.47 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:28.09 +49:20:11.4: 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 00:06:05.70 +53:15:52.3: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:28.09 +49:20:11.4: 13.55 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.36
Forced photometry filter KEPT candidate at 23:25:28.09 +49:20:11.4: ref_mag=13.55 +/- 0.36 new_mean_mag=11.7163 delta=1.84 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:05.70 +53:15:52.3: 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 23:28:27.39 +53:49:28.8: 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 23:28:27.39 +53:49:28.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:53.66 +51:59:43.1: 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 00:04:53.66 +51:59:43.1: 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 23:42:14.39 +51:45:07.7: 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 23:42:14.39 +51:45:07.7: 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 23:48:21.53 +57:40:36.0: 11.30 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:48:21.53 +57:40:36.0: 11.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.16 +/- 0.03
Forced photometry filter REJECTED candidate at 23:48:21.53 +57:40:36.0: ref_mag=11.16 +/- 0.03 new_mean_mag=11.7881 delta=-0.62 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:08:18.49 +54:03:27.9: 11.19 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:18.49 +54:03:27.9: 10.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.02
Forced photometry filter REJECTED candidate at 00:08:18.49 +54:03:27.9: ref_mag=11.02 +/- 0.02 new_mean_mag=11.7917 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 00:07:01.35 +57:49:51.0: 12.57 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:01.35 +57:49:51.0: 12.38 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.09
Forced photometry filter REJECTED candidate at 00:07:01.35 +57:49:51.0: ref_mag=12.47 +/- 0.09 new_mean_mag=11.9527 delta=0.52 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:12.85 +55:59:48.0: 8.16 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:18:38.34 +56:24:55.5: 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 23:44:12.85 +55:59:48.0: 7.86 +/- 0.00 detection
Forced photometry reference-image weighted average: 7.99 +/- 0.00
Forced photometry filter REJECTED candidate at 23:44:12.85 +55:59:48.0: ref_mag=7.99 +/- 0.00 new_mean_mag=12.2231 delta=-4.23 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:48.38 +55:58:11.8: 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 00:18:38.34 +56:24:55.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:28.71 +51:57:40.0: 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 23:53:48.38 +55:58:11.8: 11.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.05
Forced photometry filter REJECTED candidate at 23:53:48.38 +55:58:11.8: ref_mag=12.02 +/- 0.05 new_mean_mag=12.1693 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:28.71 +51:57:40.0: 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 23:26:01.28 +49:55:46.3: 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 23:26:01.28 +49:55:46.3: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:11.95 +50:00:12.0: 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 23:21:11.95 +50:00:12.0: 13.47 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out219245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236992.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): 109s
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: 50s
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Considering the candidate 235416_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235416_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235422_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235422_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235428_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235428_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:55:23.10 +56:30:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235448_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235448_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235450_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235450_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235452_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235452_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235461_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235461_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235469_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235469_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235473_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235473_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235480_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235480_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235484_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235484_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:50:48.44 +54:44:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235502_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235502_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235503_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235503_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235508_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235508_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235510_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235510_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235518_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235518_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235520_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235520_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:56:55.55 +55:04:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235521_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235521_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235525_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235525_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235531_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235531_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235535_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235535_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235537_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235537_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:08:36.80 +55:38:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235543_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235543_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235547_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235547_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235552_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235552_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235568_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235568_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235572_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235572_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235574_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235574_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235577_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235577_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:08:33.66 +56:46:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235578_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235578_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 235585_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235585_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:37:32.62 +52:48:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235586_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235586_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:48:17.69 +53:25:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235603_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235603_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235606_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235606_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:29:40.21 +57:40:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235607_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235607_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235619_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235619_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235623_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235623_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235625_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235625_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235627_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235627_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235632_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235632_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235633_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235633_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235636_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235636_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:26:42.55 +54:33:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235640_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235640_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235642_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235642_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235648_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235648_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 235650_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235650_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235653_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235653_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235655_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235655_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235656_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235656_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235658_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235658_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:31:44.65 +54:09:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235667_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235667_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235668_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235668_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235670_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235670_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235671_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235671_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:04:21.87 +51:49:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235674_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235674_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:21:22.47 +54:40:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235677_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235677_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
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Considering the candidate 235678_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235678_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:57:16.11 +56:30:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235679_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235679_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235680_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235680_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:37:09.98 +56:33:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235684_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235684_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235685_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235685_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:57:55.49 +56:42:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235688_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235688_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:29:10.62 +56:40:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235689_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235689_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235691_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235691_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235692_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235692_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:27:36.35 +55:43:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235694_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235694_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235699_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235699_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:56:59.66 +56:44:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235703_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235703_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:14:15.40 +54:02:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235707_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235707_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:51:56.92 +54:36:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235727_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235727_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:37:43.41 +55:54:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235729_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235729_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235730_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235730_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:00:21.24 +56:03:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235733_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235733_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:21:46.96 +54:49:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235734_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235734_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235735_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235735_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 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 235736_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235736_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:46:28.72 +55:12:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235750_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235750_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235751_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235751_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235753_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235753_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 235754_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 235754_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235757_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 235757_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:46:46.54 +51:02:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236034_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236034_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236063_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236063_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:13:11.29 +57:10:46.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236070_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236070_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:23:03.45 +55:45:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236091_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236091_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:43:56.54 +56:20:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236112_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236112_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:26:21.53 +53:45:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236123_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236123_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:54:36.35 +57:28:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236126_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236126_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:47:14.62 +57:25:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236134_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236134_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:18:49.79 +54:33:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236148_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236148_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236190_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236190_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:12:28.13 +57:05:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236191_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236191_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:25:37.28 +53:21:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236207_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236207_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
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Considering the candidate 236211_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236211_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236237_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236237_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:26:20.80 +56:46:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236260_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236260_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:02:36.45 +55:35:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236267_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236267_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236277_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236277_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236287_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236287_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:57:59.44 +50:26:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236302_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236302_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:10:29.02 +49:51:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236305_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236305_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:41:07.25 +51:33:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236320_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236320_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:13:37.52 +56:24:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236328_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236328_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:31:44.10 +55:25:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236340_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236340_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:23:25.81 +55:49:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236354_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236354_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
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Considering the candidate 236359_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236359_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:58:51.59 +54:42:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236361_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236361_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:43:18.32 +50:54:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236365_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236365_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:16:20.66 +53:35:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236368_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236368_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:49:47.12 +56:38:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236370_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236370_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236377_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236377_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236378_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236378_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:27:19.52 +49:58:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236386_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236386_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 236414_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236414_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:56:31.99 +53:44:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236416_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236416_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236418_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236418_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:43:15.38 +51:56:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236419_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236419_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:57:52.41 +56:27:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236420_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236420_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:33:30.63 +52:42:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236429_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236429_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:24:57.81 +53:01:59.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236437_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236437_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:28:41.72 +55:35:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236443_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236443_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:22:55.54 +51:01:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236446_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236446_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
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Considering the candidate 236452_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236452_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:33:33.47 +52:09:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236454_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236454_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:18:03.88 +49:50:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236461_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236461_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:33:03.29 +52:02:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236462_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236462_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:22:20.70 +52:13:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236467_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236467_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:57:58.25 +50:27:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236470_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236470_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236478_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236478_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236482_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236482_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:35:18.95 +50:19:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236485_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236485_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236486_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236486_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:59:00.30 +53:16:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236497_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236497_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236501_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236501_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:38:44.12 +56:37:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236508_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236508_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:00:23.14 +56:50:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236511_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236511_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:13:02.96 +49:56:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236513_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236513_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:55:15.68 +50:14:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236520_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236520_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:28:20.91 +54:48:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236530_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236530_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:52:01.87 +50:05:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236532_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236532_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:29:50.12 +54:38:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236539_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236539_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:31:40.52 +54:09:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236544_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236544_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
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Considering the candidate 236545_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236545_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:17:38.20 +51:56:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236551_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236551_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:04:15.24 +54:16:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236552_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236552_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:20:12.44 +50:06:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236563_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236563_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:32:34.90 +54:04:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236569_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236569_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:14:01.15 +55:16:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236575_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236575_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:34:07.99 +51:35:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236582_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236582_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:32:59.19 +57:36:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236583_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236583_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:46:49.15 +57:26:51.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236584_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236584_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236585_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236585_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:47:42.07 +56:52:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236589_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236589_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:48:26.65 +54:40:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236595_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236595_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:08:01.97 +53:40:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236597_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236597_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:37:53.36 +50:55:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236602_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236602_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:18:54.31 +53:18:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236606_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236606_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 236610_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236610_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
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Considering the candidate 236611_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236611_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
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Considering the candidate 236612_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236612_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:11:49.45 +54:49:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236613_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236613_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236615_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236615_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:50:23.40 +54:12:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236622_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236622_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236634_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236634_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:08:28.30 +54:42:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236652_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236652_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236664_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236664_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:20:15.60 +57:50:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236669_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236669_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236677_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236677_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:24:30.85 +56:57:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236689_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236689_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:44:49.23 +50:34:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236697_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236697_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:40:53.36 +54:25:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236712_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236712_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236719_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236719_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:54:44.67 +53:43:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236723_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236723_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:55:07.15 +56:11:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236727_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236727_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:02:27.00 +54:33:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236735_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236735_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
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Considering the candidate 236737_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236737_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:51:00.04 +54:43:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236753_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236753_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:22:46.26 +56:26:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236762_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236762_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
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Considering the candidate 236767_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236767_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:12:07.29 +53:36:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236789_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236789_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:02:24.83 +55:25:32.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236815_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236815_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:14:16.57 +56:52:52.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236833_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236833_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:01:49.61 +52:51:52.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236845_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236845_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236907_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236907_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:03:28.66 +55:39:07.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236917_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236917_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236928_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236928_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:51:28.10 +51:30:30.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236939_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236939_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236956_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236956_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236970_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 236970_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236992_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 236992_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219245_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 219245_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219159_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 219159_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:27:11.43 +53:53:44.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46841_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 46841_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:09:36.49 +51:34:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191364_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 191364_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:59:54.29 +56:58:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
Preparing report for the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179100_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 179100_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:15:50.67 +57:32:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197606_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 197606_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 23:44:31.91 +56:34:50.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64302_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111
The candidate 64302_fd_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111 did not pass the final checks
**** FOUND 00:02:27.13 +52:33:52.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 164s
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 ####
23:26:01.28 +49:55:46.3
23:43:36.04 +52:28:00.5
23:53:54.31 +51:24:50.5
00:12:16.50 +51:27:00.4
23:41:11.48 +57:06:44.9
00:04:07.71 +56:06:31.4
23:23:45.48 +55:35:38.4
23:43:58.89 +55:38:49.6
00:01:47.63 +56:08:37.0
00:07:14.46 +56:13:57.1
23:46:15.08 +52:45:11.3
23:40:15.74 +52:16:46.3
23:45:47.77 +57:16:14.9
23:31:48.19 +56:54:17.7
23:37:08.58 +50:09:11.0
23:44:34.18 +53:02:54.6
23:47:35.26 +55:28:20.1
23:39:31.92 +55:18:14.6
23:33:37.46 +53:41:37.4
00:20:11.75 +53:51:53.3
00:03:07.81 +50:05:54.2
23:23:22.55 +53:36:20.0
00:00:37.81 +56:39:40.2
23:18:18.62 +56:19:03.0
23:54:46.56 +55:01:23.6
23:19:10.07 +50:19:12.1
23:57:47.11 +56:40:12.2
23:19:10.58 +56:55:23.4
23:12:47.09 +54:51:26.3
23:12:15.21 +56:31:11.3
00:19:06.08 +56:05:28.6
23:35:27.57 +55:35:10.2
00:14:56.88 +55:03:50.8
00:07:20.94 +55:34:40.6
23:41:40.67 +53:02:02.0
23:28:57.55 +51:01:10.4
23:14:10.71 +54:09:43.9
23:18:16.20 +51:58:43.0
00:30:31.21 +55:56:24.7
23:49:49.43 +54:19:20.5
23:46:36.44 +51:42:14.8
23:21:14.36 +55:23:13.6
23:36:32.76 +50:40:33.6
23:50:25.79 +49:51:13.8
23:27:26.44 +49:36:03.6
00:15:19.60 +53:12:02.7
00:03:30.72 +53:19:18.5
23:23:03.72 +55:52:05.9
23:29:11.99 +53:11:19.5
23:59:13.16 +53:28:26.4
23:25:04.90 +55:05:34.6
23:21:39.15 +55:10:51.5
23:57:13.73 +56:42:29.5
23:56:52.56 +52:09:35.1
23:34:32.76 +49:44:28.9
23:19:31.93 +55:36:24.0
23:41:49.92 +54:40:26.7
23:12:17.78 +57:05:09.1
23:34:08.29 +54:02:57.0
23:29:23.95 +51:39:58.1
23:25:28.09 +49:20:11.4
00:06:05.70 +53:15:52.3
23:28:27.39 +53:49:28.8
00:04:53.66 +51:59:43.1
23:42:14.39 +51:45:07.7
00:18:38.34 +56:24:55.5
23:16:28.71 +51:57:40.0
23:21:11.95 +50:00:12.0
########### Completed Cas-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
23:43:36.04 +52:28:00.5
23:53:54.31 +51:24:50.5
00:12:16.50 +51:27:00.4
23:41:11.48 +57:06:44.9
00:04:07.71 +56:06:31.4
23:23:45.48 +55:35:38.4
23:43:58.89 +55:38:49.6
00:01:47.63 +56:08:37.0
00:07:14.46 +56:13:57.1
23:46:15.08 +52:45:11.3
23:40:15.74 +52:16:46.3
23:45:47.77 +57:16:14.9
23:31:48.19 +56:54:17.7
23:37:08.58 +50:09:11.0
23:44:34.18 +53:02:54.6
23:47:35.26 +55:28:20.1
23:39:31.92 +55:18:14.6
23:33:37.46 +53:41:37.4
00:20:11.75 +53:51:53.3
00:03:07.81 +50:05:54.2
23:23:22.55 +53:36:20.0
00:00:37.81 +56:39:40.2
23:18:18.62 +56:19:03.0
23:54:46.56 +55:01:23.6
23:19:10.07 +50:19:12.1
23:57:47.11 +56:40:12.2
23:19:10.58 +56:55:23.4
23:12:47.09 +54:51:26.3
23:12:15.21 +56:31:11.3
00:19:06.08 +56:05:28.6
23:35:27.57 +55:35:10.2
00:14:56.88 +55:03:50.8
00:07:20.94 +55:34:40.6
23:41:40.67 +53:02:02.0
23:28:57.55 +51:01:10.4
23:14:10.71 +54:09:43.9
23:18:16.20 +51:58:43.0
00:30:31.21 +55:56:24.7
23:49:49.43 +54:19:20.5
23:46:36.44 +51:42:14.8
23:21:14.36 +55:23:13.6
23:36:32.76 +50:40:33.6
23:50:25.79 +49:51:13.8
23:27:26.44 +49:36:03.6
00:15:19.60 +53:12:02.7
00:03:30.72 +53:19:18.5
23:23:03.72 +55:52:05.9
23:29:11.99 +53:11:19.5
23:59:13.16 +53:28:26.4
23:25:04.90 +55:05:34.6
23:21:39.15 +55:10:51.5
23:57:13.73 +56:42:29.5
23:56:52.56 +52:09:35.1
23:34:32.76 +49:44:28.9
23:19:31.93 +55:36:24.0
23:41:49.92 +54:40:26.7
23:12:17.78 +57:05:09.1
23:34:08.29 +54:02:57.0
23:29:23.95 +51:39:58.1
23:25:28.09 +49:20:11.4
00:06:05.70 +53:15:52.3
23:28:27.39 +53:49:28.8
00:04:53.66 +51:59:43.1
23:42:14.39 +51:45:07.7
00:18:38.34 +56:24:55.5
23:16:28.71 +51:57:40.0
23:26:01.28 +49:55:46.3
23:21:11.95 +50:00:12.0
###################################################################################
23:43:36.04 +52:28:00.5 -- not an asteroid (will add it to exclusion list)
23:53:54.31 +51:24:50.5 -- not an asteroid (will add it to exclusion list)
00:12:16.50 +51:27:00.4 -- not an asteroid (will add it to exclusion list)
23:41:11.48 +57:06:44.9 -- not an asteroid (will add it to exclusion list)
00:04:07.71 +56:06:31.4 -- not an asteroid (will add it to exclusion list)
23:23:45.48 +55:35:38.4 -- not an asteroid (will add it to exclusion list)
23:43:58.89 +55:38:49.6 -- not an asteroid (will add it to exclusion list)
00:01:47.63 +56:08:37.0 -- not an asteroid (will add it to exclusion list)
00:07:14.46 +56:13:57.1 -- not an asteroid (will add it to exclusion list)
23:46:15.08 +52:45:11.3 -- not an asteroid (will add it to exclusion list)
23:40:15.74 +52:16:46.3 -- not an asteroid (will add it to exclusion list)
23:45:47.77 +57:16:14.9 -- not an asteroid (will add it to exclusion list)
23:31:48.19 +56:54:17.7 -- not an asteroid (will add it to exclusion list)
23:37:08.58 +50:09:11.0 -- not an asteroid (will add it to exclusion list)
23:44:34.18 +53:02:54.6 -- not an asteroid (will add it to exclusion list)
23:47:35.26 +55:28:20.1 -- not an asteroid (will add it to exclusion list)
23:39:31.92 +55:18:14.6 -- not an asteroid (will add it to exclusion list)
23:33:37.46 +53:41:37.4 -- not an asteroid (will add it to exclusion list)
00:20:11.75 +53:51:53.3 -- not an asteroid (will add it to exclusion list)
00:03:07.81 +50:05:54.2 -- not an asteroid (will add it to exclusion list)
23:23:22.55 +53:36:20.0 -- not an asteroid (will add it to exclusion list)
00:00:37.81 +56:39:40.2 -- not an asteroid (will add it to exclusion list)
23:18:18.62 +56:19:03.0 -- not an asteroid (will add it to exclusion list)
23:54:46.56 +55:01:23.6 -- not an asteroid (will add it to exclusion list)
23:19:10.07 +50:19:12.1 -- not an asteroid (will add it to exclusion list)
23:57:47.11 +56:40:12.2 -- not an asteroid (will add it to exclusion list)
23:19:10.58 +56:55:23.4 -- not an asteroid (will add it to exclusion list)
23:12:47.09 +54:51:26.3 -- not an asteroid (will add it to exclusion list)
23:12:15.21 +56:31:11.3 -- not an asteroid (will add it to exclusion list)
00:19:06.08 +56:05:28.6 -- not an asteroid (will add it to exclusion list)
23:35:27.57 +55:35:10.2 -- not an asteroid (will add it to exclusion list)
00:14:56.88 +55:03:50.8 -- not an asteroid (will add it to exclusion list)
00:07:20.94 +55:34:40.6 -- not an asteroid (will add it to exclusion list)
23:41:40.67 +53:02:02.0 -- not an asteroid (will add it to exclusion list)
23:28:57.55 +51:01:10.4 -- not an asteroid (will add it to exclusion list)
23:14:10.71 +54:09:43.9 -- not an asteroid (will add it to exclusion list)
23:18:16.20 +51:58:43.0 -- not an asteroid (will add it to exclusion list)
00:30:31.21 +55:56:24.7 -- not an asteroid (will add it to exclusion list)
23:49:49.43 +54:19:20.5 -- not an asteroid (will add it to exclusion list)
23:46:36.44 +51:42:14.8 -- not an asteroid (will add it to exclusion list)
23:21:14.36 +55:23:13.6 -- not an asteroid (will add it to exclusion list)
23:36:32.76 +50:40:33.6 -- not an asteroid (will add it to exclusion list)
23:50:25.79 +49:51:13.8 -- not an asteroid (will add it to exclusion list)
23:27:26.44 +49:36:03.6 -- not an asteroid (will add it to exclusion list)
00:15:19.60 +53:12:02.7 -- not an asteroid (will add it to exclusion list)
00:03:30.72 +53:19:18.5 -- not an asteroid (will add it to exclusion list)
23:23:03.72 +55:52:05.9 -- not an asteroid (will add it to exclusion list)
23:29:11.99 +53:11:19.5 -- not an asteroid (will add it to exclusion list)
23:59:13.16 +53:28:26.4 -- not an asteroid (will add it to exclusion list)
23:25:04.90 +55:05:34.6 -- not an asteroid (will add it to exclusion list)
23:21:39.15 +55:10:51.5 -- not an asteroid (will add it to exclusion list)
23:57:13.73 +56:42:29.5 -- not an asteroid (will add it to exclusion list)
23:56:52.56 +52:09:35.1 -- not an asteroid (will add it to exclusion list)
23:34:32.76 +49:44:28.9 -- not an asteroid (will add it to exclusion list)
23:19:31.93 +55:36:24.0 -- not an asteroid (will add it to exclusion list)
23:41:49.92 +54:40:26.7 -- not an asteroid (will add it to exclusion list)
23:12:17.78 +57:05:09.1 -- not an asteroid (will add it to exclusion list)
23:34:08.29 +54:02:57.0 -- not an asteroid (will add it to exclusion list)
23:29:23.95 +51:39:58.1 -- not an asteroid (will add it to exclusion list)
23:25:28.09 +49:20:11.4 -- not an asteroid (will add it to exclusion list)
00:06:05.70 +53:15:52.3 -- not an asteroid (will add it to exclusion list)
23:28:27.39 +53:49:28.8 -- not an asteroid (will add it to exclusion list)
00:04:53.66 +51:59:43.1 -- not an asteroid (will add it to exclusion list)
23:42:14.39 +51:45:07.7 -- not an asteroid (will add it to exclusion list)
00:18:38.34 +56:24:55.5 -- not an asteroid (will add it to exclusion list)
23:16:28.71 +51:57:40.0 -- not an asteroid (will add it to exclusion list)
23:26:01.28 +49:55:46.3 -- not an asteroid (will add it to exclusion list)
23:21:11.95 +50:00:12.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:37.81 +56:39:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:47.63 +56:08:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:07.81 +50:05:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:30.72 +53:19:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:07.71 +56:06:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:53.66 +51:59:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:05.70 +53:15:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:14.46 +56:13:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:20.94 +55:34:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:16.50 +51:27:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:56.88 +55:03:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:19.60 +53:12:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:38.34 +56:24:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:06.08 +56:05:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:11.75 +53:51:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:31.21 +55:56:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:15.21 +56:31:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:17.78 +57:05:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:47.09 +54:51:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:10.71 +54:09:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:28.71 +51:57:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:16.20 +51:58:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:18.62 +56:19:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:10.07 +50:19:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:10.58 +56:55:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:31.93 +55:36:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:11.95 +50:00:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:14.36 +55:23:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:39.15 +55:10:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:03.72 +55:52:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:22.55 +53:36:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:45.48 +55:35:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:04.90 +55:05:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:28.09 +49:20:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:01.28 +49:55:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:26.44 +49:36:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:27.39 +53:49:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:57.55 +51:01:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:11.99 +53:11:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:23.95 +51:39:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:48.19 +56:54:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:37.46 +53:41:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:08.29 +54:02:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:32.76 +49:44:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:27.57 +55:35:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:32.76 +50:40:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:08.58 +50:09:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:31.92 +55:18:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:15.74 +52:16:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:11.48 +57:06:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:40.67 +53:02:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:49.92 +54:40:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:14.39 +51:45:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:36.04 +52:28:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:58.89 +55:38:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:34.18 +53:02:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:47.77 +57:16:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:15.08 +52:45:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:36.44 +51:42:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:35.26 +55:28:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:49.43 +54:19:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:25.79 +49:51:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:54.31 +51:24:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:46.56 +55:01:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:52.56 +52:09:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:13.73 +56:42:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:47.11 +56:40:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:13.16 +53:28:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:00:37.81 +56:39:40.2 -- not a known variable star
00:01:47.63 +56:08:37.0 -- not a known variable star
00:03:07.81 +50:05:54.2 -- not a known variable star
00:03:30.72 +53:19:18.5 -- a known variable star
00:04:07.71 +56:06:31.4 -- not a known variable star
00:04:53.66 +51:59:43.1 -- not a known variable star
00:06:05.70 +53:15:52.3 -- not a known variable star
00:07:14.46 +56:13:57.1 -- not a known variable star
00:07:20.94 +55:34:40.6 -- not a known variable star
00:12:16.50 +51:27:00.4 -- a known variable star
00:14:56.88 +55:03:50.8 -- not a known variable star
00:15:19.60 +53:12:02.7 -- a known variable star
00:18:38.34 +56:24:55.5 -- a known variable star
00:19:06.08 +56:05:28.6 -- not a known variable star
00:20:11.75 +53:51:53.3 -- not a known variable star
00:30:31.21 +55:56:24.7 -- a known variable star
23:12:15.21 +56:31:11.3 -- not a known variable star
23:12:17.78 +57:05:09.1 -- not a known variable star
23:12:47.09 +54:51:26.3 -- not a known variable star
23:14:10.71 +54:09:43.9 -- not a known variable star
23:16:28.71 +51:57:40.0 -- not a known variable star
23:18:16.20 +51:58:43.0 -- not a known variable star
23:18:18.62 +56:19:03.0 -- not a known variable star
23:19:10.07 +50:19:12.1 -- not a known variable star
23:19:10.58 +56:55:23.4 -- not a known variable star
23:19:31.93 +55:36:24.0 -- not a known variable star
23:21:11.95 +50:00:12.0 -- a known variable star
23:21:14.36 +55:23:13.6 -- not a known variable star
23:21:39.15 +55:10:51.5 -- not a known variable star
23:23:03.72 +55:52:05.9 -- not a known variable star
23:23:22.55 +53:36:20.0 -- not a known variable star
23:23:45.48 +55:35:38.4 -- not a known variable star
23:25:04.90 +55:05:34.6 -- not a known variable star
23:25:28.09 +49:20:11.4 -- not a known variable star
23:26:01.28 +49:55:46.3 -- a known variable star
23:27:26.44 +49:36:03.6 -- a known variable star
23:28:27.39 +53:49:28.8 -- not a known variable star
23:28:57.55 +51:01:10.4 -- not a known variable star
23:29:11.99 +53:11:19.5 -- not a known variable star
23:29:23.95 +51:39:58.1 -- not a known variable star
23:31:48.19 +56:54:17.7 -- not a known variable star
23:33:37.46 +53:41:37.4 -- not a known variable star
23:34:08.29 +54:02:57.0 -- a known variable star
23:34:32.76 +49:44:28.9 -- not a known variable star
23:35:27.57 +55:35:10.2 -- not a known variable star
23:36:32.76 +50:40:33.6 -- not a known variable star
23:37:08.58 +50:09:11.0 -- not a known variable star
23:39:31.92 +55:18:14.6 -- not a known variable star
23:40:15.74 +52:16:46.3 -- not a known variable star
23:41:11.48 +57:06:44.9 -- not a known variable star
23:41:40.67 +53:02:02.0 -- a known variable star
23:41:49.92 +54:40:26.7 -- not a known variable star
23:42:14.39 +51:45:07.7 -- not a known variable star
23:43:36.04 +52:28:00.5 -- a known variable star
23:43:58.89 +55:38:49.6 -- not a known variable star
23:44:34.18 +53:02:54.6 -- not a known variable star
23:45:47.77 +57:16:14.9 -- not a known variable star
23:46:15.08 +52:45:11.3 -- not a known variable star
23:46:36.44 +51:42:14.8 -- not a known variable star
23:47:35.26 +55:28:20.1 -- not a known variable star
23:49:49.43 +54:19:20.5 -- not a known variable star
23:50:25.79 +49:51:13.8 -- not a known variable star
23:53:54.31 +51:24:50.5 -- not a known variable star
23:54:46.56 +55:01:23.6 -- not a known variable star
23:56:52.56 +52:09:35.1 -- not a known variable star
23:57:13.73 +56:42:29.5 -- not a known variable star
23:57:47.11 +56:40:12.2 -- not a known variable star
23:59:13.16 +53:28:26.4 -- a known variable star
Found 56 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
68 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 68 (excluding asteroids and hot pixels, 56 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)2461243.68098924 -observatory V36
07:07:36.46 +18:07:37.6 Mercury (2.5mag)
10:59:32.26 +07:14:47.4 Venus (-4.2mag)
04:59:13.19 +22:39:45.6 Mars (1.3mag)
08:27:27.55 +19:36:15.2 Jupiter (-1.8mag)
00:56:42.98 +03:22:19.7 Saturn (0.7mag)
04:09:20.50 +20:50:41.7 Uranus (5.8mag)
00:16:50.04 +00:18:47.0 Neptune (7.7mag)
20:29:47.73 -23:23:11.0 Pluto (14.4mag)
14:10:17.17 -19:04:39.9 Moon (-10.6mag)
-rw-r--r-- 1 apache apache 362 Jul 22 00:17 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461243.68098924:
08:27:23.58 +19:36:32.2 Io (6.0mag)
08:27:37.00 +19:35:37.7 Europa (6.3mag)
08:27:16.49 +19:37:02.2 Ganymede (5.6mag)
08:27:31.80 +19:36:03.5 Callisto (6.7mag)
08:25:29.29 +19:25:55.7 Himalia (15.7mag)
08:27:30.42 +19:36:04.6 Thebe (16.6mag)
08:24:51.38 +19:27:51.1 Elara (17.7mag)
08:31:18.97 +19:24:10.2 Pasiphae (17.9mag)
08:31:43.58 +19:43:11.5 Carme (19.0mag)
00:56:37.04 +03:22:47.2 Titan (8.5mag)
00:56:46.59 +03:22:22.2 Rhea (9.8mag)
00:56:11.54 +03:19:47.5 Iapetus (11.2mag)
00:56:42.37 +03:21:41.0 Hyperion (14.5mag)
00:56:27.89 +03:17:50.9 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 22 00:17 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461243.68098924:
18:08:01.26 -29:56:37.4 JWST
18:46:43.54 +20:23:02.9 Chandra
19:57:12.46 +20:03:27.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 22 00:17 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461243.68098924 -observatory V36
02:52:35.48 +15:45:43.0 17.8mag P/1996 R2 (Lagerkvist)
18:09:37.09 -34:35:55.0 13.8mag P/2010 H2 (Vales)
06:37:25.95 -68:22:30.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:04:47.23 +32:39:22.4 17.6mag C/2017 K2 (PANSTARRS)
02:44:54.64 +25:50:36.9 15.9mag P/2021 N1 (ZTF)
22:51:48.53 +32:09:02.1 17.3mag C/2022 E2 (ATLAS)
06:25:38.70 +26:47:58.5 16.7mag C/2022 N2 (PANSTARRS)
10:05:59.13 +29:14:44.7 16.9mag C/2022 QE78 (ATLAS)
09:17:28.26 +05:11:01.3 17.9mag C/2022 R6 (PANSTARRS)
15:10:59.90 -11:41:49.4 17.8mag P/2023 B1 (PANSTARRS)
21:34:02.77 +67:20:12.0 17.9mag C/2023 H5 (Lemmon)
16:09:44.68 -11:17:28.5 14.1mag C/2023 R1 (PANSTARRS)
08:21:44.51 +66:22:52.5 18.0mag C/2024 A1 (ATLAS)
07:47:56.14 +30:34:40.2 14.9mag C/2024 E1 (Wierzchos)
15:11:19.93 +15:33:18.0 17.6mag C/2024 G6 (ATLAS)
19:25:44.51 +41:24:15.6 13.7mag C/2024 J3 (ATLAS)
21:34:08.94 +47:37:43.4 17.7mag C/2024 R4 (PANSTARRS)
05:00:34.67 -13:20:10.7 15.6mag C/2024 T5 (ATLAS)
06:44:03.96 +27:05:17.0 17.9mag C/2025 J1 (Borisov)
07:22:03.99 -14:02:39.1 17.1mag C/2025 R3 (PANSTARRS)
10:10:20.60 +21:52:58.1 17.5mag C/2025 V2 (Rankin)
12:49:11.76 +03:22:24.3 17.0mag C/2025 Y1 (ATLAS)
16:22:26.78 +79:00:50.9 17.1mag C/2026 A2 (Bok)
02:57:26.38 +45:42:32.2 16.9mag C/2026 B2 (Sun-Gao)
11:33:32.84 +06:26:45.3 17.1mag A/2026 E1
21:36:48.16 -19:46:33.9 7.0mag 10P/Tempel
11:19:20.05 -02:26:17.4 16.2mag 29P/Schwassmann-Wachmann
04:16:53.60 +30:47:59.3 17.9mag 47P/Ashbrook-Jackson
10:32:41.25 +10:12:26.2 17.1mag 63P/Wild
00:52:30.45 -05:03:52.2 15.5mag 65P/Gunn
04:55:49.53 +20:38:25.5 13.7mag 78P/Gehrels
02:40:17.59 +12:06:07.8 16.4mag 88P/Howell
07:09:58.02 +29:38:15.6 15.9mag 93P/Lovas
04:59:50.01 +31:19:02.6 16.6mag 114P/Wiseman-Skiff
08:37:32.61 +29:15:11.6 15.1mag 123P/West-Hartley
11:10:27.02 -03:35:11.9 16.9mag 124P/Mrkos
05:10:32.82 +21:04:49.4 16.2mag 128P/Shoemaker-Holt
05:58:16.95 +19:31:41.2 17.8mag 131P/Mueller
07:54:44.13 +14:20:59.1 17.0mag 141P-D/Machholz
03:21:19.89 -20:29:48.4 14.9mag 161P/Hartley-IRAS
06:15:44.97 +36:07:10.4 15.5mag 162P/SidingSpring
18:21:15.55 +23:47:00.9 13.7mag 169P/NEAT
02:08:21.54 +08:43:46.5 17.6mag 220P/McNaught
16:35:54.32 -08:57:31.2 17.3mag 235P/LINEAR
20:35:14.20 -51:45:07.8 17.8mag 259P/Garradd
02:32:45.86 +17:36:03.0 15.5mag 260P/McNaught
06:13:20.54 +37:34:11.6 17.3mag 295P/LINEAR
15:06:50.88 +04:56:25.1 17.6mag 391P/Kowalski
08:45:18.56 +19:10:30.2 17.9mag 450P/LONEOS
08:10:09.15 +38:13:06.9 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.4K Jul 22 00:17 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -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
04:50:01.03 -02:22:33.80 2026-07-16.17 17.02
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
-rw-r--r-- 1 apache apache 189K Jul 22 00:16 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:10:20.128 -14:09:55.94 AT 2026tgt 2026-07-09.29 23.278
23:20:06.593 -16:17:48.29 AT 2026tgs 2026-07-09.35 22.6556
19:05:03.872 -23:19:36.91 AT 2026tgr 2026-07-09.23 21.5848
19:15:04.585 -19:48:18.27 AT 2026tgq 2026-07-09.23 23.246
20:21:03.786 -12:05:37.19 AT 2026tgp 2026-07-09.24 23.8773
23:08:13.178 -10:15:07.93 AT 2026tgo 2026-07-09.35 22.4826
00:37:15.628 -45:39:35.39 AT 2026tgn 2026-07-09.41 23.2909
20:54:32.460 -21:42:36.81 AT 2026tgm 2026-07-07.32 22.7357
20:34:11.836 -23:17:26.34 AT 2026tgl 2026-07-07.33 23.0469
20:17:45.315 -09:54:20.41 AT 2026tgk 2026-07-07.33 23.0751
20:23:26.444 -13:44:06.33 AT 2026tgj 2026-07-07.33 22.0545
21:14:51.004 -20:43:30.25 AT 2026tgi 2026-07-07.32 23.2188
22:38:49.833 -08:33:48.30 AT 2026tgh 2026-07-07.42 23.1231
20:32:39.725 -23:08:39.00 AT 2026tgg 2026-07-07.33 22.1838
22:45:39.123 -09:28:10.17 AT 2026tgf 2026-07-07.42 22.453
20:21:52.213 -13:12:29.72 AT 2026tge 2026-07-07.33 22.0452
20:21:15.623 -26:24:20.31 AT 2026tgd 2026-07-07.33 22.44
20:49:27.325 -20:47:19.83 AT 2026tgc 2026-07-07.32 23.1686
20:33:36.615 -22:45:24.14 AT 2026tgb 2026-07-07.33 22.9236
21:35:21.131 -20:17:56.65 AT 2026tga 2026-07-07.43 21.3752
-rw-r--r-- 1 apache apache 88K Jul 22 00:16 tns_transients_list.txt
