This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9
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 08 02.1592 2461254.6592 11.66 23:41:58.54 +57:29:43.2
113.67841 -4.12311 galactic Cas Second-epoch detections are separated by 1.3" and 9.5 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 1998675164486065792 | 23:41:59.29 +57:29:16.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.585+/-0.044 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:58.54 +57:29:43.2: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:41:58.54 +57:29:43.2: 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 08 02.1592* 23 41 58.54 +57 29 43.2 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998675164486065792,2461254.6592,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998675164486065792 20260802.1592 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.41 23:39:32.15 +55:18:31.3
112.75668 -6.13619 galactic Cas Second-epoch detections are separated by 2.9" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:39:32.15 +55:18:31.3 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.349+/-0.040 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:32.15 +55:18:31.3: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:39:32.15 +55:18:31.3: 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 08 02.1592* 23 39 32.15 +55 18 31.3 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461254.6592,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260802.1592 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.21 23:19:17.12 +52:37:38.6
109.06125 -7.74481 galactic And Second-epoch detections are separated by 4.7" and 10.0 pix
The object was found in VSX18" Gaia DR3 1992593800028520576
Type: ROT
# Max. Min./Amp. JD0 Period
13.530 G 13.570 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:17.12 +52:37:38.6: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:17.12 +52:37:38.6: 13.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 19 17.12 +52 37 38.6 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992593800028520576,2461254.6592,11.21,0.05,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
Gaia DR3 1992593800028520576 20260802.1592 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 08 02.1592 2461254.6592 11.31 23:16:55.85 +55:40:35.4
109.82493 -4.77167 galactic Cas Second-epoch detections are separated by 0.8" and 10.0 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 J349.2418+55.6751 | 23:16:59.12 +55:40:23.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.648+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:55.85 +55:40:35.4: 13.55 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:16:55.85 +55:40:35.4: 13.62 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.55 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 16 55.85 +55 40 35.4 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 J349.2418+55.6751,2461254.6592,11.31,0.05,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
ATO J349.2418+55.6751 20260802.1592 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 08 02.1592 2461254.6592 11.29 23:12:41.10 +54:49:15.0
108.94549 -5.34682 galactic Cas Second-epoch detections are separated by 1.5" and 10.2 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 1996494626770732160 | 23:12:37.83 +54:49:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:41.10 +54:49:15.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:12:41.10 +54:49:15.0: 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 08 02.1592* 23 12 41.10 +54 49 15.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996494626770732160,2461254.6592,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996494626770732160 20260802.1592 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.09 23:17:51.00 +50:50:41.0
108.21156 -9.33265 galactic And Second-epoch detections are separated by 2.3" and 10.0 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 | 23:17:51.00 +50:50:41.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.775+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:51.00 +50:50:41.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:51.00 +50:50:41.0: 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 08 02.1592* 23 17 51.00 +50 50 41.0 11.1 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
target,2461254.6592,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260802.1592 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.07 23:13:36.11 +55:20:57.5
109.26495 -4.90494 galactic Cas Second-epoch detections are separated by 1.8" and 10.3 pix
The object was found in VSX 3" Gaia DR3 1996708378701541632
Type: VAR
# Max. Min./Amp. JD0 Period
13.040 G 13.100 G 0.017762900000 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 23:13:36.11 +55:20:57.5: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:13:36.11 +55:20:57.5: 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 08 02.1592* 23 13 36.11 +55 20 57.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996708378701541632,2461254.6592,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996708378701541632 20260802.1592 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.10 23:28:23.02 +57:13:13.6
111.84076 -3.85196 galactic Cas Second-epoch detections are separated by 0.1" and 9.7 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 1998829370990757376 | 23:28:25.30 +57:13:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.453+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:23.02 +57:13:13.6: 13.46 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:23.02 +57:13:13.6: 13.73 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 28 23.02 +57 13 13.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998829370990757376,2461254.6592,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998829370990757376 20260802.1592 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.04 23:27:35.79 +56:17:57.1
111.44458 -4.69115 galactic Cas Second-epoch detections are separated by 0.7" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1997045374712242560 | 23:27:36.33 +56:17:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.605+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:35.79 +56:17:57.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:35.79 +56:17:57.1: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 27 35.79 +56 17 57.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997045374712242560,2461254.6592,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997045374712242560 20260802.1592 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.95 23:34:15.89 +55:29:02.3
112.08609 -5.75428 galactic Cas Second-epoch detections are separated by 0.4" and 9.6 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 1997472294465069312 | 23:34:19.47 +55:28:58.8 (Gaia DR3) | DSCT/GDOR (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 23:34:15.89 +55:29:02.3: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:15.89 +55:29:02.3: 13.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 34 15.89 +55 29 02.3 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 1997472294465069312,2461254.6592,10.95,0.05,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 1997472294465069312 20260802.1592 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 08 02.1592 2461254.6592 11.10 23:29:28.48 +54:41:00.3
111.18444 -6.30807 galactic Cas Second-epoch detections are separated by 2.1" and 9.7 pix
The object was found in VSX11" Gaia DR3 1995868454895136896
Type: ROT
# Max. Min./Amp. JD0 Period
16.960 G 17.020 G K
ATTENTION: measured mag 11.10 is 5.9 mag brighter than the VSX record maximum brightness 16.96 - 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 23:29:28.48 +54:41:00.3: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:29:28.48 +54:41:00.3: 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 08 02.1592* 23 29 28.48 +54 41 00.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995868454895136896,2461254.6592,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995868454895136896 20260802.1592 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.04 23:20:50.50 +57:13:03.5
110.87413 -3.51789 galactic Cas Second-epoch detections are separated by 1.2" and 9.7 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 2009382964622103680 | 23:20:48.14 +57:12:33.4 (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 23:20:50.50 +57:13:03.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:20:50.50 +57:13:03.5: 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 08 02.1592* 23 20 50.50 +57 13 03.5 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 2009382964622103680,2461254.6592,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009382964622103680 20260802.1592 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.16 23:18:56.56 +53:20:38.9
109.26687 -7.05575 galactic Cas Second-epoch detections are separated by 0.7" and 10.1 pix
The object was found in VSX 1" Gaia DR3 1995687275993223168
Type: ROT
# Max. Min./Amp. JD0 Period
12.980 G 13.010 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.56 +53:20:38.9: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:18:56.56 +53:20:38.9: 13.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 18 56.56 +53 20 38.9 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995687275993223168,2461254.6592,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995687275993223168 20260802.1592 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.97 23:14:46.43 +55:59:23.9
109.65542 -4.36989 galactic Cas Second-epoch detections are separated by 1.9" and 9.9 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 | 23:14:46.43 +55:59:23.9 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.036 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:46.43 +55:59:23.9: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:14:46.43 +55:59:23.9: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 14 46.43 +55 59 23.9 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
target,2461254.6592,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260802.1592 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.80 23:34:11.85 +56:47:43.9
112.46604 -4.49847 galactic Cas Second-epoch detections are separated by 1.0" and 9.5 pix
The object was found in VSX 0" Gaia DR3 1998538721964108416
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.860 G 12.920 G 0.595710000000 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 23:34:11.85 +56:47:43.9: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:11.85 +56:47:43.9: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 34 11.85 +56 47 43.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998538721964108416,2461254.6592,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998538721964108416 20260802.1592 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.02 23:17:35.72 +54:08:15.3
109.36234 -6.24319 galactic Cas Second-epoch detections are separated by 0.2" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J349.4060+54.1166 | 23:17:37.25 +54:07:40.8 (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 23:17:35.72 +54:08:15.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:35.72 +54:08:15.3: 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 08 02.1592* 23 17 35.72 +54 08 15.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.4060+54.1166,2461254.6592,11.02,0.05,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 J349.4060+54.1166 20260802.1592 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 08 02.1592 2461254.6592 10.96 23:20:43.26 +52:38:33.1
109.27261 -7.80663 galactic And Second-epoch detections are separated by 1.4" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.1805+52.6425 | 23:20:44.38 +52:38:46.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.334+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:43.26 +52:38:33.1: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:20:43.26 +52:38:33.1: 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 08 02.1592* 23 20 43.26 +52 38 33.1 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.1805+52.6425,2461254.6592,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.1805+52.6425 20260802.1592 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 9.96 00:23:08.15 +54:41:30.5
118.80966 -7.95326 galactic Cas Second-epoch detections are separated by 1.7" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 419667134313546880 | 00:23:06.28 +54:42:11.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.223+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:08.15 +54:41:30.5: 13.58 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:23:08.15 +54:41:30.5: 13.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.58 +/- 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 08 02.1592* 00 23 08.15 +54 41 30.5 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419667134313546880,2461254.6592,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419667134313546880 20260802.1592 9.96CV 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 08 02.1592 2461254.6592 10.79 23:21:14.61 +55:23:14.2
110.29692 -5.25632 galactic Cas Second-epoch detections are separated by 1.4" and 9.6 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 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 23:21:14.61 +55:23:14.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:14.61 +55:23:14.2: 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 08 02.1592* 23 21 14.61 +55 23 14.2 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 1996852414723764608,2461254.6592,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996852414723764608 20260802.1592 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.45 23:37:54.66 +52:32:04.1
111.74153 -8.73241 galactic Cas Second-epoch detections are separated by 2.0" and 9.6 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 J354.4870+52.5413 | 23:37:56.31 +52:32:16.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.573+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:54.66 +52:32:04.1: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:37:54.66 +52:32:04.1: 13.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 37 54.66 +52 32 04.1 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
ATO J354.4870+52.5413,2461254.6592,10.45,0.05,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 J354.4870+52.5413 20260802.1592 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.78 23:17:08.66 +56:21:20.3
110.09633 -4.14805 galactic Cas Second-epoch detections are separated by 0.6" and 9.8 pix
The object was found in VSX 2" Gaia DR3 2009204534508637824
Type: ROT
# Max. Min./Amp. JD0 Period
12.700 G 12.740 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:08.66 +56:21:20.3: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:08.66 +56:21:20.3: 13.46 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 17 08.66 +56 21 20.3 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 2009204534508637824,2461254.6592,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009204534508637824 20260802.1592 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.18 23:42:50.97 +52:40:01.2
112.50790 -8.81101 galactic Cas Second-epoch detections are separated by 0.1" and 9.7 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 1993025220904837760 | 23:42:48.42 +52:39:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.736+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:50.97 +52:40:01.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:42:50.97 +52:40:01.2: 13.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 42 50.97 +52 40 01.2 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993025220904837760,2461254.6592,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993025220904837760 20260802.1592 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.30 23:31:08.95 +54:16:09.0
111.28770 -6.77737 galactic Cas Second-epoch detections are separated by 0.7" and 9.7 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 | Large-amplitude variable Gaia DR2 1994340477332018432 | 23:31:09.41 +54:16:29.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.319+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:08.95 +54:16:09.0: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:31:08.95 +54:16:09.0: 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 08 02.1592* 23 31 08.95 +54 16 09.0 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1994340477332018432,2461254.6592,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1994340477332018432 20260802.1592 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.31 23:17:30.38 +52:15:02.5
108.67043 -8.00080 galactic And Second-epoch detections are separated by 1.1" and 10.0 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 J349.3943+52.2449 | 23:17:32.34 +52:15:07.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.181+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:30.38 +52:15:02.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:30.38 +52:15:02.5: 13.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 17 30.38 +52 15 02.5 10.3 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 J349.3943+52.2449,2461254.6592,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.3943+52.2449 20260802.1592 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.11 23:25:10.72 +52:02:46.6
109.71584 -8.59817 galactic And Second-epoch detections are separated by 0.7" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1991670210261865600 | 23:25:09.10 +52:02:29.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.675+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:10.72 +52:02:46.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:10.72 +52:02:46.6: 13.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 25 10.72 +52 02 46.6 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
Gaia DR3 1991670210261865600,2461254.6592,10.11,0.05,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 1991670210261865600 20260802.1592 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 9.61 23:18:36.08 +54:06:28.4
109.49039 -6.32323 galactic Cas Second-epoch detections are separated by 0.8" and 10.1 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 1995956450184696320 | 23:18:38.53 +54:06:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956PMcCO..13a....B AG+53 1640 J-Ks=0.296+/-0.026 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:36.08 +54:06:28.4: 12.23 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:18:36.08 +54:06:28.4: 12.36 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.29 +/- 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 08 02.1592* 23 18 36.08 +54 06 28.4 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995956450184696320,2461254.6592,9.61,0.05,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 1995956450184696320 20260802.1592 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 08 02.1592 2461254.6592 9.38 23:21:37.66 +55:42:58.6
110.46113 -4.96573 galactic Cas Second-epoch detections are separated by 0.4" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1997000745714549504 | 23:21:40.22 +55:42:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-0.027 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:37.66 +55:42:58.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:37.66 +55:42:58.6: 13.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 21 37.66 +55 42 58.6 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997000745714549504,2461254.6592,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997000745714549504 20260802.1592 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.48 23:27:06.64 +56:40:01.5
111.49903 -4.32116 galactic Cas Second-epoch detections are separated by 2.5" and 9.4 pix
The object was not found in VSX
The object was found in ASASSN-V 0" ASASSN-V J232706.67+564001.6
Type: L
MeanMag 12.94 m Amp. 0.12 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 23:27:06.64 +56:40:01.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:06.64 +56:40:01.5: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 27 06.64 +56 40 01.5 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461254.6592,10.48,0.05,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
VARIABLE_NAME 20260802.1592 10.48CV 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 08 02.1592 2461254.6592 10.02 00:26:18.98 +56:47:25.5
119.47856 -5.91279 galactic Cas Second-epoch detections are separated by 3.2" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.5721+56.7854 | 00:26:19.27 +56:47:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:18.98 +56:47:25.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:26:18.98 +56:47:25.5: 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 08 02.1592* 00 26 18.98 +56 47 25.5 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J006.5721+56.7854,2461254.6592,10.02,0.05,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
ATO J006.5721+56.7854 20260802.1592 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 08 02.1592 2461254.6592 10.71 23:24:57.21 +55:06:10.1
110.70111 -5.70197 galactic Cas Second-epoch detections are separated by 1.9" and 9.5 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 J351.2448+55.0966 | 23:24:57.21 +55:06:10.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.373+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:57.21 +55:06:10.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:24:57.21 +55:06:10.1: 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 08 02.1592* 23 24 57.21 +55 06 10.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.2448+55.0966,2461254.6592,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.2448+55.0966 20260802.1592 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.64 23:26:19.29 +51:13:15.1
109.61033 -9.43596 galactic Cas Second-epoch detections are separated by 0.1" and 10.0 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 1991384509038443904 | 23:26:16.19 +51:12:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:19.29 +51:13:15.1: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:19.29 +51:13:15.1: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 26 19.29 +51 13 15.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991384509038443904,2461254.6592,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991384509038443904 20260802.1592 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.83 23:22:36.38 +57:23:00.6
111.15519 -3.44300 galactic Cas Second-epoch detections are separated by 3.6" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2009390970447326080 | 23:22:32.69 +57:22:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:36.38 +57:23:00.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:36.38 +57:23:00.6: 13.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 22 36.38 +57 23 00.6 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 2009390970447326080,2461254.6592,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009390970447326080 20260802.1592 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.86 23:25:57.98 +53:09:48.4
110.20113 -7.58253 galactic Cas Second-epoch detections are separated by 0.9" and 9.9 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 J351.4851+53.1640 | 23:25:57.98 +53:09:48.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.104+/-0.028 (A)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:57.98 +53:09:48.4: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:57.98 +53:09:48.4: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 25 57.98 +53 09 48.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.4851+53.1640,2461254.6592,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.4851+53.1640 20260802.1592 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.04 23:11:36.37 +56:08:18.1
109.29894 -4.06809 galactic Cas Second-epoch detections are separated by 1.4" and 10.1 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 J347.9024+56.1427 | 23:11:36.19 +56:08:18.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.185+/-0.043 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:36.37 +56:08:18.1: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:11:36.37 +56:08:18.1: 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 08 02.1592* 23 11 36.37 +56 08 18.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.9024+56.1427,2461254.6592,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.9024+56.1427 20260802.1592 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.03 23:26:31.98 +54:58:42.3
110.87520 -5.89346 galactic Cas Second-epoch detections are separated by 3.9" and 10.4 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 J351.6404+54.9646 | 23:26:36.73 +54:58:23.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1927AnHar.100...33C HD 236120 J-Ks=0.591+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:31.98 +54:58:42.3: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:31.98 +54:58:42.3: 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 08 02.1592* 23 26 31.98 +54 58 42.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.6404+54.9646,2461254.6592,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.6404+54.9646 20260802.1592 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 08 02.1592 2461254.6592 10.60 00:06:47.68 +54:28:39.2
116.41351 -7.82820 galactic Cas Second-epoch detections are separated by 1.1" and 9.4 pix
The object was found in VSX 6" Gaia DR3 420384840525796224
Type: ROT
# Max. Min./Amp. JD0 Period
13.210 G 13.250 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 00:06:47.68 +54:28:39.2: 13.50 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:06:47.68 +54:28:39.2: 13.66 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.50 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 00 06 47.68 +54 28 39.2 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420384840525796224,2461254.6592,10.60,0.05,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 420384840525796224 20260802.1592 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.92 23:28:46.89 +52:18:46.6
110.33163 -8.52498 galactic Cas Second-epoch detections are separated by 1.3" and 10.0 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 1991700068875645312 | 23:28:50.45 +52:18:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.468+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:46.89 +52:18:46.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:46.89 +52:18:46.6: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 28 46.89 +52 18 46.6 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 1991700068875645312,2461254.6592,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991700068875645312 20260802.1592 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.02 23:23:03.56 +55:52:07.8
110.70301 -4.89032 galactic Cas Second-epoch detections are separated by 2.2" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 23:23:03.56 +55:52:07.8: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:03.56 +55:52:07.8: 13.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 23 03.56 +55 52 07.8 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+55.8722,2461254.6592,11.02,0.05,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 20260802.1592 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 08 02.1592 2461254.6592 11.16 23:25:04.78 +55:05:34.9
110.71500 -5.71714 galactic Cas Second-epoch detections are separated by 1.0" and 10.0 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 | 23:25:04.78 +55:05:34.9 (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 23:25:04.78 +55:05:34.9: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:04.78 +55:05:34.9: 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 08 02.1592* 23 25 04.78 +55 05 34.9 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461254.6592,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260802.1592 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.02 23:28:27.08 +51:42:39.4
110.08892 -9.07947 galactic Cas Second-epoch detections are separated by 0.8" and 10.0 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 1991589086918724480 | 23:28:26.77 +51:42:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.798+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:27.08 +51:42:39.4: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:27.08 +51:42:39.4: 13.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 28 27.08 +51 42 39.4 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 1991589086918724480,2461254.6592,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991589086918724480 20260802.1592 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 08 02.1592 2461254.6592 11.27 23:27:31.99 +51:51:35.2
110.00111 -8.89294 galactic Cas Second-epoch detections are separated by 0.7" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1991607778616239616 | 23:27:28.10 +51:51:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.318+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:31.99 +51:51:35.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:31.99 +51:51:35.2: 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 08 02.1592* 23 27 31.99 +51 51 35.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991607778616239616,2461254.6592,11.27,0.05,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
Gaia DR3 1991607778616239616 20260802.1592 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 08 02.1592 2461254.6592 10.87 23:47:55.55 +51:49:46.2
113.05142 -9.81966 galactic Cas Second-epoch detections are separated by 0.7" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1945024185367145216 | 23:47:58.83 +51:50:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.719+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:55.55 +51:49:46.2: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:47:55.55 +51:49:46.2: 13.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 47 55.55 +51 49 46.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1945024185367145216,2461254.6592,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1945024185367145216 20260802.1592 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.13 23:17:12.14 +52:50:30.1
108.84066 -7.43250 galactic And Second-epoch detections are separated by 4.6" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:17:12.14 +52:50:30.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:12.14 +52:50:30.1: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:12.14 +52:50:30.1: 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 08 02.1592* 23 17 12.14 +52 50 30.1 11.1 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
target,2461254.6592,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260802.1592 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.17 23:34:22.94 +53:50:20.4
111.61268 -7.33068 galactic Cas Second-epoch detections are separated by 2.5" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1994092400019847168 | 23:34:27.25 +53:50:36.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.360+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:22.94 +53:50:20.4: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:22.94 +53:50:20.4: 13.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 34 22.94 +53 50 20.4 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994092400019847168,2461254.6592,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994092400019847168 20260802.1592 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.88 23:51:39.01 +53:05:09.5
113.91467 -8.73582 galactic Cas Second-epoch detections are separated by 0.3" and 9.5 pix
The object was found in VSX18" Gaia DR3 1945388604754909568
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.730 G 15.780 G 0.048264400000 A
ATTENTION: measured mag 10.88 is 4.8 mag brighter than the VSX record maximum brightness 15.73 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:39.01 +53:05:09.5: 13.35 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:51:39.01 +53:05:09.5: 13.41 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 51 39.01 +53 05 09.5 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 1945388604754909568,2461254.6592,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1945388604754909568 20260802.1592 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.06 00:07:11.42 +57:23:34.3
116.97484 -4.96622 galactic Cas Second-epoch detections are separated by 1.7" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.7977+57.3855 | 00:07:11.42 +57:23:34.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:11.42 +57:23:34.3: 13.36 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:07:11.42 +57:23:34.3: 13.54 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.36 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 00 07 11.42 +57 23 34.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.7977+57.3855,2461254.6592,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.7977+57.3855 20260802.1592 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.07 23:58:05.48 +56:28:01.3
115.57515 -5.64082 galactic Cas Second-epoch detections are separated by 1.3" and 9.4 pix
The object was found in VSX 1" ASASSN-V J235805.40+562800.5
Type: YSO
# Max. Min./Amp. JD0 Period
13.410 V 13.540 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:05.48 +56:28:01.3: 12.36 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:58:05.48 +56:28:01.3: 12.54 +/- 0.22 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 58 05.48 +56 28 01.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235805.40+562800.5,2461254.6592,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J235805.40+562800.5 20260802.1592 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.26 23:23:47.39 +54:34:22.6
110.36546 -6.14622 galactic Cas Second-epoch detections are separated by 1.1" and 9.7 pix
The object was found in VSX 2" ZTF J232347.55+543421.8
Type: SR
# Max. Min./Amp. JD0 Period
12.954 r Y 0.042 r 2458657.89370 34.975481300000
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 23:23:47.39 +54:34:22.6: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:47.39 +54:34:22.6: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 23 47.39 +54 34 22.6 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
ZTF J232347.55+543421.8,2461254.6592,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J232347.55+543421.8 20260802.1592 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.47 23:21:38.87 +55:10:54.8
110.28069 -5.46901 galactic Cas Second-epoch detections are separated by 1.3" and 9.9 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 J350.4212+55.1780 | 23:21:38.87 +55:10:54.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.679+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:38.87 +55:10:54.8: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:38.87 +55:10:54.8: 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 08 02.1592* 23 21 38.87 +55 10 54.8 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 J350.4212+55.1780,2461254.6592,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.4212+55.1780 20260802.1592 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 11.48 23:19:32.11 +55:36:24.4
110.14520 -4.96672 galactic Cas Second-epoch detections are separated by 3.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 23:19:32.11 +55:36:24.4: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:32.11 +55:36:24.4: 13.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 19 32.11 +55 36 24.4 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
Gaia DR3 1996916972372159360,2461254.6592,11.48,0.05,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 1996916972372159360 20260802.1592 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 08 02.1592 2461254.6592 11.45 23:25:19.25 +53:20:34.4
110.16856 -7.38134 galactic Cas Second-epoch detections are separated by 2.2" and 9.9 pix
The object was found in VSX 2" Gaia DR3 1992733987761271680
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.250 G 13.270 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 23:25:19.25 +53:20:34.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:19.25 +53:20:34.4: 13.68 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 25 19.25 +53 20 34.4 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 1992733987761271680,2461254.6592,11.45,0.05,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
Gaia DR3 1992733987761271680 20260802.1592 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 08 02.1592 2461254.6592 11.39 23:47:38.58 +53:30:03.6
113.42750 -8.18939 galactic Cas Second-epoch detections are separated by 2.5" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.9165+53.5145 | 23:47:41.36 +53:30:31.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.988+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:38.58 +53:30:03.6: 13.53 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:47:38.58 +53:30:03.6: 13.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.53 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 47 38.58 +53 30 03.6 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 J356.9165+53.5145,2461254.6592,11.39,0.05,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
ATO J356.9165+53.5145 20260802.1592 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 08 02.1592 2461254.6592 11.65 23:36:48.34 +54:33:54.8
112.16745 -6.73923 galactic Cas Second-epoch detections are separated by 3.5" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1994315566520904064 | 23:36:44.27 +54:33:41.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.797+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:48.34 +54:33:54.8: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:36:48.34 +54:33:54.8: 13.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 36 48.34 +54 33 54.8 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994315566520904064,2461254.6592,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994315566520904064 20260802.1592 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 02.1592 2461254.6592 10.03 23:52:16.33 +54:38:46.5
114.36815 -7.23875 galactic Cas Second-epoch detections are separated by 0.3" and 9.5 pix
The object was found in VSX 2" V1464 Cas
Type: SRB
# Max. Min./Amp. JD0 Period
12.540 V 13.640 V 2458298.20850 149.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:16.33 +54:38:46.5: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:52:16.33 +54:38:46.5: 13.85 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 52 16.33 +54 38 46.5 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1464 Cas,2461254.6592,10.03,0.05,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
V1464 Cas 20260802.1592 10.03CV 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 08 02.1592 2461254.6592 10.92 23:57:19.02 +54:52:46.4
115.13533 -7.17084 galactic Cas Second-epoch detections are separated by 6.0" and 8.4 pix
The object was found in VSX 5" LP Cas
Type: M
# Max. Min./Amp. JD0 Period
14.900 pg < 17.000 pg 2429143.00000 294.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:19.02 +54:52:46.4: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:57:19.02 +54:52:46.4: 13.71 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 02.1592* 23 57 19.02 +54 52 46.4 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
LP Cas,2461254.6592,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LP Cas 20260802.1592 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461254.65961214 02.08.2026 03:49:40.489 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 20369
Objects passed selection criteria: 20257
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 13974.8
Average stars matched: 13627.2 (97.5134 %)
Memory usage VmPeak: 247168 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 1 22:57:54 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: 2461254.65961214 02.08.2026 03:49:40.489 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 140
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: 459 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 155125
Objects passed selection criteria: 154680
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 115936
Average stars matched: 111645 (96.2988 %)
Memory usage VmPeak: 628236 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 1 23:06:50 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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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: 2461254.65887863
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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits'
wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits'
wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
Image size: 938.2'x624.1' 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: 00:00:40.021 +53:59:19.72 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 00:00:40.021 +53:59:19.72
Angular distance between the image centers 0.1082 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
Image size: 938.2'x624.1' 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: 00:00:44.315 +53:58:38.13 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 00:00:44.315 +53:58:38.13
Angular distance between the image centers 0.1218 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 00:00:40.021 +53:59:19.72
Second-epoch second image center 00:00:44.315 +53:58:38.13
Angular distance between the image centers 0.01562 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.rMVdBzz978
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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits &> /tmp/tmp.Wld2IClCt2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits &> /tmp/tmp.5Gr3cvi2Zt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits &> /tmp/tmp.CcKhpFPakJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0821 to 14.9840 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 345.0821 to 14.9840 deg, Dec 48.2682 to 59.2677 deg
Loaded 25149 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 25149 matchable stars (28951 detected on the reference image) matched the Tycho-2 photometric calibration catalog (0.21%) - 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)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0821 to 14.9840 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 345.0821 to 14.9840 deg, Dec 48.2682 to 59.2677 deg
Loaded 25149 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: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=6.3)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28570 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0823 to 14.9843 deg, Dec +48.2680 to +59.2686 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 345.0823 to 14.9843 deg, Dec 48.2680 to 59.2686 deg
Loaded 25151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 53 out of 62 total matches.
Matched with Tycho-2 62 out of 28570 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 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
2.4 pix Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
Limiting magnitude estimates:
14.9 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
14.9 mag. Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
13.4 mag. fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
13.4 mag. fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.7 (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.rMVdBzz978 (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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2748, bad_region=6855, passed=28951
Got 28951 stars (including 19826 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 28951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3491 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2179 matched stars entering correct_measured_positions(), 2402 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2040 matched stars entering correct_measured_positions(), 23307 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.92"
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 345.0820 through 0 to 15.0032, gap 15.0032 to 345.0820
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3563 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2451 matched stars entering correct_measured_positions(), 23308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.07"
Accuracy estimation diagnostic: 2380 matched stars entering correct_measured_positions(), 23397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.12"
Excluding outliers - 2380 stars left (next iteration limit 2244)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=2380 sigma_overall_arcsec=12.078 sigma_q1_arcsec=29.329 sigma_q2_arcsec=29.014 sigma_q3_arcsec=5.984 sigma_q4_arcsec=5.684 n_q1=514 n_q2=285 n_q3=882 n_q4=699 worst_quadrant_to_overall_ratio=2.428
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.Wld2IClCt2 (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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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_05-10-10_20.00sec_4.90C_LIGHT_0469.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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_05-10-10_20.00sec_4.90C_LIGHT_0469.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_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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=2755, bad_region=6825, passed=28570
Got 28570 stars (including 19480 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat
util/solve_plate_with_UCAC5 got 28570 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 345.0823 through 0 to 14.9843, gap 14.9843 to 345.0823
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3497 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2173 matched stars entering correct_measured_positions(), 2402 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2035 matched stars entering correct_measured_positions(), 22970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.99"
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 345.0792 through 0 to 15.0034, gap 15.0034 to 345.0792
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3582 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2451 matched stars entering correct_measured_positions(), 22971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.15"
Accuracy estimation diagnostic: 2378 matched stars entering correct_measured_positions(), 23037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.01"
Excluding outliers - 2378 stars left (next iteration limit 2238)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits N_match=2378 sigma_overall_arcsec=11.840 sigma_q1_arcsec=29.033 sigma_q2_arcsec=28.890 sigma_q3_arcsec=5.697 sigma_q4_arcsec=5.199 n_q1=506 n_q2=300 n_q3=879 n_q4=693 worst_quadrant_to_overall_ratio=2.452
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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.5Gr3cvi2Zt (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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.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_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.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=395, bad_region=1000, passed=7353
Got 7353 stars (including 5997 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat
util/solve_plate_with_UCAC5 got 7353 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3275 through 0 to 14.8396, gap 14.8396 to 345.3275
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 4891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 6616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 345.3271 through 0 to 14.8401, gap 14.8401 to 345.3271
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 6616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 6616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4893 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4893 robust_rms=5.687 arcsec worst_quadrant_rms=13.351 arcsec
SIP_REFIT: SIP order 3 trial: matched=4893 robust_rms=0.648 arcsec worst_quadrant_rms=0.680 arcsec
SIP_REFIT: SIP order 5 trial: matched=4893 robust_rms=0.570 arcsec worst_quadrant_rms=0.624 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4893 robust_rms_before=0.782 arcsec robust_rms_before_corrected=0.532 arcsec robust_rms_after=0.570 arcsec worst_quadrant_rms_before=0.549 worst_quadrant_rms_after=0.624
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.549 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits N_match=4893 sigma_overall_arcsec=0.530 sigma_q1_arcsec=0.538 sigma_q2_arcsec=0.486 sigma_q3_arcsec=0.543 sigma_q4_arcsec=0.541 n_q1=1643 n_q2=639 n_q3=1819 n_q4=792 worst_quadrant_to_overall_ratio=1.024
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.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.CcKhpFPakJ (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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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=394, bad_region=1026, passed=7101
Got 7101 stars (including 5722 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat
util/solve_plate_with_UCAC5 got 7101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3279 through 0 to 14.8388, gap 14.8388 to 345.3279
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.2)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 4893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 345.3273 through 0 to 14.8392, gap 14.8392 to 345.3273
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.2)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 6310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 6310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4893 stars left (next iteration limit 5381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4893 robust_rms=5.487 arcsec worst_quadrant_rms=14.504 arcsec
SIP_REFIT: SIP order 3 trial: matched=4893 robust_rms=0.627 arcsec worst_quadrant_rms=0.666 arcsec
SIP_REFIT: SIP order 5 trial: matched=4893 robust_rms=0.571 arcsec worst_quadrant_rms=0.616 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4893 robust_rms_before=0.793 arcsec robust_rms_before_corrected=0.531 arcsec robust_rms_after=0.571 arcsec worst_quadrant_rms_before=0.540 worst_quadrant_rms_after=0.616
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.540 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits N_match=4893 sigma_overall_arcsec=0.538 sigma_q1_arcsec=0.545 sigma_q2_arcsec=0.488 sigma_q3_arcsec=0.552 sigma_q4_arcsec=0.572 n_q1=1636 n_q2=623 n_q3=1851 n_q4=783 worst_quadrant_to_overall_ratio=1.064
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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=12.078 worst_q_ratio=2.428
ref2=Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits sigma_overall=11.840 worst_q_ratio=2.452
new1=fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits sigma_overall=0.530 worst_q_ratio=1.024
new2=fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits sigma_overall=0.538 worst_q_ratio=1.064
reference average sigma_overall=11.959 worst_q_ratio=2.44
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 (2380 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 11.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469_astrometric_residuals.png (2378 matched stars from wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 10.68 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082_astrometric_residuals.png (4893 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083_astrometric_residuals.png (4893 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07077_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 07077_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:09:36.44 +51:34:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21482_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 21482_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:31.85 +56:34:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06239_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 06239_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:58:25.18 +51:23:24.3 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
Image size: 938.2'x624.1' 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: 00:00:40.021 +53:59:19.72 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 00:00:40.021 +53:59:19.72
Angular distance between the image centers 0.1082 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
Image size: 938.2'x624.1' 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: 00:00:44.315 +53:58:38.13 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 00:00:44.315 +53:58:38.13
Angular distance between the image centers 0.1218 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 00:00:40.021 +53:59:19.72
Second-epoch second image center 00:00:44.315 +53:58:38.13
Angular distance between the image centers 0.01562 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.nN1Za3pIjj
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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits &> /tmp/tmp.DMGRm4oRxI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits &> /tmp/tmp.7jI9dvPSn0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits &> /tmp/tmp.nLaCT3eS3o
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0121 to 15.0290 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 345.0121 to 15.0290 deg, Dec 48.2503 to 59.2677 deg
Loaded 25285 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 25285 matchable stars (200953 detected on the reference image) matched the Tycho-2 photometric calibration catalog (0.41%) - 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)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0121 to 15.0290 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 345.0121 to 15.0290 deg, Dec 48.2503 to 59.2677 deg
Loaded 25285 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: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=4.7)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 201615 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0124 to 15.0290 deg, Dec +48.2304 to +59.2696 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 345.0124 to 15.0290 deg, Dec 48.2304 to 59.2696 deg
Loaded 25320 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): 108 out of 156 total matches.
Matched with Tycho-2 156 out of 201615 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 103 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_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
Limiting magnitude estimates:
13.2 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
13.2 mag. Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
11.7 mag. fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
11.7 mag. fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
All-image limiting magnitude estimate: 11.7 (SNR ) 11.3 (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.nN1Za3pIjj (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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=60, blended=29230, bad_region=30798, passed=200893
Got 200893 stars (including 144443 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 200893 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3471 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2133 matched stars entering correct_measured_positions(), 2388 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1977 matched stars entering correct_measured_positions(), 177569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.93"
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 345.0078 through 0 to 15.0480, gap 15.0480 to 345.0078
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3545 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2435 matched stars entering correct_measured_positions(), 177569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.94"
Accuracy estimation diagnostic: 2366 matched stars entering correct_measured_positions(), 177773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.34"
Excluding outliers - 2366 stars left (next iteration limit 2174)
SIP_REFIT: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=2366 sigma_overall_arcsec=12.864 sigma_q1_arcsec=27.379 sigma_q2_arcsec=28.581 sigma_q3_arcsec=5.692 sigma_q4_arcsec=5.485 n_q1=495 n_q2=335 n_q3=832 n_q4=704 worst_quadrant_to_overall_ratio=2.222
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.DMGRm4oRxI (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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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_05-10-10_20.00sec_4.90C_LIGHT_0469.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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_05-10-10_20.00sec_4.90C_LIGHT_0469.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_05-10-10_20.00sec_4.90C_LIGHT_0469.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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=75, blended=29046, bad_region=30736, passed=201540
Got 201540 stars (including 145414 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat
util/solve_plate_with_UCAC5 got 201540 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 345.0124 through 0 to 15.0290, gap 15.0290 to 345.0124
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3461 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2151 matched stars entering correct_measured_positions(), 2382 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.83"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2004 matched stars entering correct_measured_positions(), 178188 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.18"
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 345.0090 through 0 to 15.0476, gap 15.0476 to 345.0090
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 3528 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2399 matched stars entering correct_measured_positions(), 178188 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.20"
Accuracy estimation diagnostic: 2347 matched stars entering correct_measured_positions(), 178165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.57"
Excluding outliers - 2347 stars left (next iteration limit 2204)
SIP_REFIT: wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits N_match=2347 sigma_overall_arcsec=13.542 sigma_q1_arcsec=27.752 sigma_q2_arcsec=27.788 sigma_q3_arcsec=5.911 sigma_q4_arcsec=5.028 n_q1=482 n_q2=338 n_q3=848 n_q4=679 worst_quadrant_to_overall_ratio=2.052
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.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.7jI9dvPSn0 (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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.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_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.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=5, blended=3919, bad_region=6233, passed=68955
Got 68955 stars (including 59100 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat
util/solve_plate_with_UCAC5 got 68955 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0087 through 0 to 14.8396, gap 14.8396 to 345.0087
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 64599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0083 through 0 to 14.8401, gap 14.8401 to 345.0083
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 64599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 64599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4904 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits N_match=4904 sigma_overall_arcsec=0.526 sigma_q1_arcsec=0.543 sigma_q2_arcsec=0.490 sigma_q3_arcsec=0.530 sigma_q4_arcsec=0.556 n_q1=1701 n_q2=631 n_q3=1767 n_q4=805 worst_quadrant_to_overall_ratio=1.056
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.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.nLaCT3eS3o (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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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=8, blended=3712, bad_region=6239, passed=68670
Got 68670 stars (including 58975 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat
util/solve_plate_with_UCAC5 got 68670 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0952 through 0 to 15.0355, gap 15.0355 to 345.0952
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 64073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0946 through 0 to 15.0359, gap 15.0359 to 345.0946
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 64073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 64073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4906 stars left (next iteration limit 5395)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits N_match=4906 sigma_overall_arcsec=0.550 sigma_q1_arcsec=0.554 sigma_q2_arcsec=0.486 sigma_q3_arcsec=0.572 sigma_q4_arcsec=0.576 n_q1=1693 n_q2=606 n_q3=1811 n_q4=796 worst_quadrant_to_overall_ratio=1.048
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-48-37_20.00sec_-0.00C_LIGHT_0082.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.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_2026-08-01_CI_Cas-04-Q2b1x1_225154_TTUQ2b1x1_926588_ao4LQGg9/wcs_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:17.12 +52:37:38.6: 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 23:41:58.54 +57:29:43.2: 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 23:39:32.15 +55:18:31.3: 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 23:12:41.10 +54:49:15.0: 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 23:16:55.85 +55:40:35.4: 13.55 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:40:09.61 +56:41:49.9: 11.87 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:36.11 +55:20:57.5: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:51.00 +50:50:41.0: 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 23:27:35.79 +56:17:57.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:23.02 +57:13:13.6: 13.46 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:39:32.15 +55:18:31.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:40:09.61 +56:41:49.9: 11.68 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:12:41.10 +54:49:15.0: 13.58 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.76 +/- 0.05
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:41:58.54 +57:29:43.2: 13.67 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:40:09.61 +56:41:49.9: ref_mag=11.76 +/- 0.05 new_mean_mag=11.2137 delta=0.54 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:17.12 +52:37:38.6: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:16:55.85 +55:40:35.4: 13.62 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.55 +/- 0.34
Forced photometry filter KEPT candidate at 23:16:55.85 +55:40:35.4: ref_mag=13.55 +/- 0.34 new_mean_mag=11.3168 delta=2.24 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:13:36.11 +55:20:57.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:51.00 +50:50:41.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:35.79 +56:17:57.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:23.02 +57:13:13.6: 13.73 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.22
Forced photometry filter KEPT candidate at 23:28:23.02 +57:13:13.6: ref_mag=13.56 +/- 0.22 new_mean_mag=11.1044 delta=2.45 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:15.89 +55:29:02.3: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:15.89 +55:29:02.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:28.48 +54:41:00.3: 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 23:20:50.50 +57:13:03.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:29:28.48 +54:41:00.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:20:50.50 +57:13:03.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.56 +53:20:38.9: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:18:56.56 +53:20:38.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:46.43 +55:59:23.9: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:14:46.43 +55:59:23.9: 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 23:34:11.85 +56:47:43.9: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:11.85 +56:47:43.9: 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 23:17:35.72 +54:08:15.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:35.72 +54:08:15.3: 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 23:20:43.26 +52:38:33.1: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:08.15 +54:41:30.5: 13.58 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:20:43.26 +52:38:33.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:14.61 +55:23:14.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:54.66 +52:32:04.1: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:23:08.15 +54:41:30.5: 13.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.58 +/- 0.36
Forced photometry filter KEPT candidate at 00:23:08.15 +54:41:30.5: ref_mag=13.58 +/- 0.36 new_mean_mag=9.9399 delta=3.64 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:14.61 +55:23:14.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:37:54.66 +52:32:04.1: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:08.66 +56:21:20.3: 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 23:42:50.97 +52:40:01.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:08.66 +56:21:20.3: 13.46 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.28
Forced photometry filter KEPT candidate at 23:17:08.66 +56:21:20.3: ref_mag=13.46 +/- 0.28 new_mean_mag=10.7615 delta=2.70 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:42:50.97 +52:40:01.2: 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 23:31:08.95 +54:16:09.0: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:31:08.95 +54:16:09.0: 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 23:17:30.38 +52:15:02.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:30.38 +52:15:02.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:10.72 +52:02:46.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:10.72 +52:02:46.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:36.08 +54:06:28.4: 12.23 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:18:36.08 +54:06:28.4: 12.36 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.07
Forced photometry filter KEPT candidate at 23:18:36.08 +54:06:28.4: ref_mag=12.29 +/- 0.07 new_mean_mag=9.6037 delta=2.68 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:37.66 +55:42:58.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:37.66 +55:42:58.6: 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 23:22:37.24 +53:23:07.2: 11.15 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:37.24 +53:23:07.2: 11.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.16 +/- 0.02
Forced photometry filter REJECTED candidate at 23:22:37.24 +53:23:07.2: ref_mag=11.16 +/- 0.02 new_mean_mag=10.3243 delta=0.83 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:06.64 +56:40:01.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:06.64 +56:40:01.5: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:18.98 +56:47:25.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:26:18.98 +56:47:25.5: 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 23:24:57.21 +55:06:10.1: 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 23:26:19.29 +51:13:15.1: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:24:57.21 +55:06:10.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:19.29 +51:13:15.1: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:36.38 +57:23:00.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:22:36.38 +57:23:00.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:57.98 +53:09:48.4: 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 23:11:36.37 +56:08:18.1: 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 23:26:31.98 +54:58:42.3: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:57.98 +53:09:48.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:11:36.37 +56:08:18.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:26:31.98 +54:58:42.3: 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 00:06:47.68 +54:28:39.2: 13.50 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:06:47.68 +54:28:39.2: 13.66 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.50 +/- 0.29
Forced photometry filter KEPT candidate at 00:06:47.68 +54:28:39.2: ref_mag=13.50 +/- 0.29 new_mean_mag=10.5772 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:03.56 +55:52:07.8: 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 23:28:46.89 +52:18:46.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:03.56 +55:52:07.8: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:46.89 +52:18:46.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:56.51 +56:28:30.8: 10.52 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:57:56.51 +56:28:30.8: 10.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.02
Forced photometry filter REJECTED candidate at 23:57:56.51 +56:28:30.8: ref_mag=10.51 +/- 0.02 new_mean_mag=10.8096 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:04.78 +55:05:34.9: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:04.78 +55:05:34.9: 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 23:28:27.08 +51:42:39.4: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:28:27.08 +51:42:39.4: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:31.99 +51:51:35.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:27:31.99 +51:51:35.2: 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 23:47:55.55 +51:49:46.2: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:12.14 +52:50:30.1: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:47:55.55 +51:49:46.2: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:17:12.14 +52:50:30.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:22.94 +53:50:20.4: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:39.01 +53:05:09.5: 13.35 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:34:22.94 +53:50:20.4: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:51:39.01 +53:05:09.5: 13.41 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.17
Forced photometry filter KEPT candidate at 23:51:39.01 +53:05:09.5: ref_mag=13.38 +/- 0.17 new_mean_mag=10.8444 delta=2.54 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:11.42 +57:23:34.3: 13.36 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 00:07:11.42 +57:23:34.3: 13.54 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.36 +/- 0.31
Forced photometry filter KEPT candidate at 00:07:11.42 +57:23:34.3: ref_mag=13.36 +/- 0.31 new_mean_mag=11.0553 delta=2.30 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:05.48 +56:28:01.3: 12.36 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:58:05.48 +56:28:01.3: 12.54 +/- 0.22 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.14
Forced photometry filter KEPT candidate at 23:58:05.48 +56:28:01.3: ref_mag=12.44 +/- 0.14 new_mean_mag=11.0747 delta=1.37 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:47.39 +54:34:22.6: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:23:47.39 +54:34:22.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:38.87 +55:10:54.8: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:21:38.87 +55:10:54.8: 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 23:19:32.11 +55:36:24.4: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:19:32.11 +55:36:24.4: 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 23:25:19.25 +53:20:34.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:25:19.25 +53:20:34.4: 13.68 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.33
Forced photometry filter KEPT candidate at 23:25:19.25 +53:20:34.4: ref_mag=13.68 +/- 0.33 new_mean_mag=11.4482 delta=2.23 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:38.58 +53:30:03.6: 13.53 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:47:38.58 +53:30:03.6: 13.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.53 +/- 0.27
Forced photometry filter KEPT candidate at 23:47:38.58 +53:30:03.6: ref_mag=13.53 +/- 0.27 new_mean_mag=11.3827 delta=2.15 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:48.34 +54:33:54.8: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:36:48.34 +54:33:54.8: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:16.33 +54:38:46.5: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:52:16.33 +54:38:46.5: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:19.02 +54:52:46.4: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-10-10_20.00sec_4.90C_LIGHT_0469.fits at 23:57:19.02 +54:52:46.4: 13.71 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.33
Forced photometry filter KEPT candidate at 23:57:19.02 +54:52:46.4: ref_mag=13.71 +/- 0.33 new_mean_mag=10.9156 delta=2.80 (need > 0.90)
Adding exclusion_list_local.txt__out109307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227779.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 77s
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: 47s
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Considering the candidate 226894_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226894_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 226900_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226900_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 226907_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 226907_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
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Considering the candidate 226917_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 226917_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:50:37.60 +57:09:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226928_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 226928_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:21:38.39 +50:04:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226942_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 226942_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:31:44.60 +54:09:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226944_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226944_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 226945_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226945_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 226956_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226956_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
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Considering the candidate 226968_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 226968_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:45:59.24 +56:53:29.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226970_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226970_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226971_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226971_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226974_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226974_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226980_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226980_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226983_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226983_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226984_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226984_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226987_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226987_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226990_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226990_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226992_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226992_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226995_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226995_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226996_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 226996_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226998_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 226998_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:38:10.87 +52:49:02.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227001_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227001_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227006_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227006_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:59.02 +57:58:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227008_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227008_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227010_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227010_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227011_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227011_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227014_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227014_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:21:47.08 +54:49:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227015_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227015_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227018_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227018_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227019_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227019_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227020_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227020_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227021_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227021_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227022_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227022_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:39:37.66 +57:08:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227026_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227026_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:46:46.51 +51:02:02.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227027_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227027_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227110_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227110_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227214_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227214_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:11.25 +56:38:11.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227225_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227225_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227259_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227259_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227279_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227279_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:31:20.71 +49:29:52.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227293_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227293_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:42:05.61 +57:16:09.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227295_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227295_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:57:10.90 +55:43:59.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227313_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227313_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:55:17.27 +58:06:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227323_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227323_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:43:12.97 +51:57:42.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227330_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227330_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227334_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227334_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:43:56.63 +56:20:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227335_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227335_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:54:36.24 +57:28:24.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227336_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227336_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:18:49.80 +54:33:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227338_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227338_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227343_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227343_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227348_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227348_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:47:14.60 +57:25:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227349_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227349_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227358_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227358_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:59:25.74 +57:41:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227362_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227362_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:21:35.06 +50:17:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227370_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227370_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:26:21.39 +53:45:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227381_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227381_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:42:07.05 +57:15:39.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227382_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227382_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:59:23.75 +50:31:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227388_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227388_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:12:28.24 +57:05:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227393_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227393_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:15:42.84 +54:52:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227402_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227402_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227416_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227416_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227420_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227420_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227433_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227433_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227455_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227455_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:57:06.86 +55:40:48.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227461_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227461_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:25:37.11 +53:21:58.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227482_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227482_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227490_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227490_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227503_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227503_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:23:03.47 +55:45:37.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227505_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227505_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227515_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227515_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227521_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227521_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:03.96 +56:47:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227540_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227540_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227559_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227559_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227573_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227573_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227577_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227577_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227609_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227609_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:00:23.02 +56:51:49.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227646_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227646_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:36:00.64 +53:25:27.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227648_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227648_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227671_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227671_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227686_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227686_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:02:36.35 +55:35:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227693_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227693_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227694_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227694_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227705_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227705_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227709_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227709_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227725_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227725_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227731_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227731_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227758_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227758_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227766_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227766_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:58:51.71 +54:42:08.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227779_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 227779_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227793_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 227793_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:08:17.89 +52:45:56.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25587_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 25587_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:21:11.83 +50:00:13.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46841_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 46841_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:09:36.45 +51:34:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54745_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 54745_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:57:25.79 +52:02:15.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191364_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 191364_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:59:54.28 +56:58:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60942_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 60942_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:33:22.93 +52:10:37.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121532_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 121532_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:20:22.29 +54:45:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109307_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 109307_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179100_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 179100_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:15:50.61 +57:32:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113957_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
Preparing report for the candidate 113957_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197606_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 197606_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:44:31.87 +56:34:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65524_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 65524_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:11:13.11 +52:32:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46078_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083
The candidate 46078_fd_Cas-04-Q2b1x1_2026-08-01_22-49-40_20.00sec_-0.00C_LIGHT_0083 did not pass the final checks
**** FOUND 23:58:25.17 +51:23:24.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 130s
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 ####
23:52:16.33 +54:38:46.5
23:57:19.02 +54:52:46.4
23:41:58.54 +57:29:43.2
23:39:32.15 +55:18:31.3
23:19:17.12 +52:37:38.6
23:16:55.85 +55:40:35.4
23:12:41.10 +54:49:15.0
23:17:51.00 +50:50:41.0
23:13:36.11 +55:20:57.5
23:28:23.02 +57:13:13.6
23:27:35.79 +56:17:57.1
23:34:15.89 +55:29:02.3
23:29:28.48 +54:41:00.3
23:20:50.50 +57:13:03.5
23:18:56.56 +53:20:38.9
23:14:46.43 +55:59:23.9
23:34:11.85 +56:47:43.9
23:17:35.72 +54:08:15.3
23:20:43.26 +52:38:33.1
00:23:08.15 +54:41:30.5
23:21:14.61 +55:23:14.2
23:37:54.66 +52:32:04.1
23:17:08.66 +56:21:20.3
23:42:50.97 +52:40:01.2
23:31:08.95 +54:16:09.0
23:17:30.38 +52:15:02.5
23:25:10.72 +52:02:46.6
23:18:36.08 +54:06:28.4
23:21:37.66 +55:42:58.6
23:27:06.64 +56:40:01.5
00:26:18.98 +56:47:25.5
23:24:57.21 +55:06:10.1
23:26:19.29 +51:13:15.1
23:22:36.38 +57:23:00.6
23:25:57.98 +53:09:48.4
23:11:36.37 +56:08:18.1
23:26:31.98 +54:58:42.3
00:06:47.68 +54:28:39.2
23:28:46.89 +52:18:46.6
23:23:03.56 +55:52:07.8
23:25:04.78 +55:05:34.9
23:28:27.08 +51:42:39.4
23:27:31.99 +51:51:35.2
23:47:55.55 +51:49:46.2
23:17:12.14 +52:50:30.1
23:34:22.94 +53:50:20.4
23:51:39.01 +53:05:09.5
00:07:11.42 +57:23:34.3
23:58:05.48 +56:28:01.3
23:23:47.39 +54:34:22.6
23:21:38.87 +55:10:54.8
23:19:32.11 +55:36:24.4
23:25:19.25 +53:20:34.4
23:47:38.58 +53:30:03.6
23:36:48.34 +54:33:54.8
########### 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 ####
23:41:58.54 +57:29:43.2
23:39:32.15 +55:18:31.3
23:19:17.12 +52:37:38.6
23:16:55.85 +55:40:35.4
23:12:41.10 +54:49:15.0
23:17:51.00 +50:50:41.0
23:13:36.11 +55:20:57.5
23:28:23.02 +57:13:13.6
23:27:35.79 +56:17:57.1
23:34:15.89 +55:29:02.3
23:29:28.48 +54:41:00.3
23:20:50.50 +57:13:03.5
23:18:56.56 +53:20:38.9
23:14:46.43 +55:59:23.9
23:34:11.85 +56:47:43.9
23:17:35.72 +54:08:15.3
23:20:43.26 +52:38:33.1
00:23:08.15 +54:41:30.5
23:21:14.61 +55:23:14.2
23:37:54.66 +52:32:04.1
23:17:08.66 +56:21:20.3
23:42:50.97 +52:40:01.2
23:31:08.95 +54:16:09.0
23:17:30.38 +52:15:02.5
23:25:10.72 +52:02:46.6
23:18:36.08 +54:06:28.4
23:21:37.66 +55:42:58.6
23:27:06.64 +56:40:01.5
00:26:18.98 +56:47:25.5
23:24:57.21 +55:06:10.1
23:26:19.29 +51:13:15.1
23:22:36.38 +57:23:00.6
23:25:57.98 +53:09:48.4
23:11:36.37 +56:08:18.1
23:26:31.98 +54:58:42.3
00:06:47.68 +54:28:39.2
23:28:46.89 +52:18:46.6
23:23:03.56 +55:52:07.8
23:25:04.78 +55:05:34.9
23:28:27.08 +51:42:39.4
23:27:31.99 +51:51:35.2
23:47:55.55 +51:49:46.2
23:17:12.14 +52:50:30.1
23:34:22.94 +53:50:20.4
23:51:39.01 +53:05:09.5
00:07:11.42 +57:23:34.3
23:58:05.48 +56:28:01.3
23:23:47.39 +54:34:22.6
23:21:38.87 +55:10:54.8
23:19:32.11 +55:36:24.4
23:25:19.25 +53:20:34.4
23:47:38.58 +53:30:03.6
23:36:48.34 +54:33:54.8
23:52:16.33 +54:38:46.5
23:57:19.02 +54:52:46.4
###################################################################################
23:41:58.54 +57:29:43.2 -- not an asteroid (will add it to exclusion list)
23:39:32.15 +55:18:31.3 -- not an asteroid (will add it to exclusion list)
23:19:17.12 +52:37:38.6 -- not an asteroid (will add it to exclusion list)
23:16:55.85 +55:40:35.4 -- not an asteroid (will add it to exclusion list)
23:12:41.10 +54:49:15.0 -- not an asteroid (will add it to exclusion list)
23:17:51.00 +50:50:41.0 -- not an asteroid (will add it to exclusion list)
23:13:36.11 +55:20:57.5 -- not an asteroid (will add it to exclusion list)
23:28:23.02 +57:13:13.6 -- not an asteroid (will add it to exclusion list)
23:27:35.79 +56:17:57.1 -- not an asteroid (will add it to exclusion list)
23:34:15.89 +55:29:02.3 -- not an asteroid (will add it to exclusion list)
23:29:28.48 +54:41:00.3 -- not an asteroid (will add it to exclusion list)
23:20:50.50 +57:13:03.5 -- not an asteroid (will add it to exclusion list)
23:18:56.56 +53:20:38.9 -- not an asteroid (will add it to exclusion list)
23:14:46.43 +55:59:23.9 -- not an asteroid (will add it to exclusion list)
23:34:11.85 +56:47:43.9 -- not an asteroid (will add it to exclusion list)
23:17:35.72 +54:08:15.3 -- not an asteroid (will add it to exclusion list)
23:20:43.26 +52:38:33.1 -- not an asteroid (will add it to exclusion list)
00:23:08.15 +54:41:30.5 -- not an asteroid (will add it to exclusion list)
23:21:14.61 +55:23:14.2 -- not an asteroid (will add it to exclusion list)
23:37:54.66 +52:32:04.1 -- not an asteroid (will add it to exclusion list)
23:17:08.66 +56:21:20.3 -- not an asteroid (will add it to exclusion list)
23:42:50.97 +52:40:01.2 -- not an asteroid (will add it to exclusion list)
23:31:08.95 +54:16:09.0 -- not an asteroid (will add it to exclusion list)
23:17:30.38 +52:15:02.5 -- not an asteroid (will add it to exclusion list)
23:25:10.72 +52:02:46.6 -- not an asteroid (will add it to exclusion list)
23:18:36.08 +54:06:28.4 -- not an asteroid (will add it to exclusion list)
23:21:37.66 +55:42:58.6 -- not an asteroid (will add it to exclusion list)
23:27:06.64 +56:40:01.5 -- not an asteroid (will add it to exclusion list)
00:26:18.98 +56:47:25.5 -- not an asteroid (will add it to exclusion list)
23:24:57.21 +55:06:10.1 -- not an asteroid (will add it to exclusion list)
23:26:19.29 +51:13:15.1 -- not an asteroid (will add it to exclusion list)
23:22:36.38 +57:23:00.6 -- not an asteroid (will add it to exclusion list)
23:25:57.98 +53:09:48.4 -- not an asteroid (will add it to exclusion list)
23:11:36.37 +56:08:18.1 -- not an asteroid (will add it to exclusion list)
23:26:31.98 +54:58:42.3 -- not an asteroid (will add it to exclusion list)
00:06:47.68 +54:28:39.2 -- not an asteroid (will add it to exclusion list)
23:28:46.89 +52:18:46.6 -- not an asteroid (will add it to exclusion list)
23:23:03.56 +55:52:07.8 -- not an asteroid (will add it to exclusion list)
23:25:04.78 +55:05:34.9 -- not an asteroid (will add it to exclusion list)
23:28:27.08 +51:42:39.4 -- not an asteroid (will add it to exclusion list)
23:27:31.99 +51:51:35.2 -- not an asteroid (will add it to exclusion list)
23:47:55.55 +51:49:46.2 -- not an asteroid (will add it to exclusion list)
23:17:12.14 +52:50:30.1 -- not an asteroid (will add it to exclusion list)
23:34:22.94 +53:50:20.4 -- not an asteroid (will add it to exclusion list)
23:51:39.01 +53:05:09.5 -- not an asteroid (will add it to exclusion list)
00:07:11.42 +57:23:34.3 -- not an asteroid (will add it to exclusion list)
23:58:05.48 +56:28:01.3 -- not an asteroid (will add it to exclusion list)
23:23:47.39 +54:34:22.6 -- not an asteroid (will add it to exclusion list)
23:21:38.87 +55:10:54.8 -- not an asteroid (will add it to exclusion list)
23:19:32.11 +55:36:24.4 -- not an asteroid (will add it to exclusion list)
23:25:19.25 +53:20:34.4 -- not an asteroid (will add it to exclusion list)
23:47:38.58 +53:30:03.6 -- not an asteroid (will add it to exclusion list)
23:36:48.34 +54:33:54.8 -- not an asteroid (will add it to exclusion list)
23:52:16.33 +54:38:46.5 -- not an asteroid (will add it to exclusion list)
23:57:19.02 +54:52:46.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:06:47.68 +54:28:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:11.42 +57:23:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:08.15 +54:41:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:18.98 +56:47:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:36.37 +56:08:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:41.10 +54:49:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:36.11 +55:20:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:46.43 +55:59:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:55.85 +55:40:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:08.66 +56:21:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:12.14 +52:50:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:30.38 +52:15:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:35.72 +54:08:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:51.00 +50:50:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:36.08 +54:06:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:56.56 +53:20:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:17.12 +52:37:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:32.11 +55:36:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:43.26 +52:38:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:50.50 +57:13:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:14.61 +55:23:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:37.66 +55:42:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:38.87 +55:10:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:36.38 +57:23:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:03.56 +55:52:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:47.39 +54:34:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:57.21 +55:06:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:04.78 +55:05:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:10.72 +52:02:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:19.25 +53:20:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:57.98 +53:09:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:19.29 +51:13:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:31.98 +54:58:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:06.64 +56:40:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:31.99 +51:51:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:35.79 +56:17:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:23.02 +57:13:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:27.08 +51:42:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:46.89 +52:18:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:28.48 +54:41:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:08.95 +54:16:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:11.85 +56:47:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:15.89 +55:29:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:22.94 +53:50:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:48.34 +54:33:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:54.66 +52:32:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:32.15 +55:18:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:58.54 +57:29:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:50.97 +52:40:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:38.58 +53:30:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:55.55 +51:49:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:39.01 +53:05:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:16.33 +54:38:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:19.02 +54:52:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:05.48 +56:28:01.3 -- 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)
00:06:47.68 +54:28:39.2 -- a known variable star
00:07:11.42 +57:23:34.3 -- not a known variable star
00:23:08.15 +54:41:30.5 -- not a known variable star
00:26:18.98 +56:47:25.5 -- not a known variable star
23:11:36.37 +56:08:18.1 -- not a known variable star
23:12:41.10 +54:49:15.0 -- not a known variable star
23:13:36.11 +55:20:57.5 -- a known variable star
23:14:46.43 +55:59:23.9 -- not a known variable star
23:16:55.85 +55:40:35.4 -- not a known variable star
23:17:08.66 +56:21:20.3 -- a known variable star
23:17:12.14 +52:50:30.1 -- not a known variable star
23:17:30.38 +52:15:02.5 -- not a known variable star
23:17:35.72 +54:08:15.3 -- not a known variable star
23:17:51.00 +50:50:41.0 -- not a known variable star
23:18:36.08 +54:06:28.4 -- not a known variable star
23:18:56.56 +53:20:38.9 -- a known variable star
23:19:17.12 +52:37:38.6 -- a known variable star
23:19:32.11 +55:36:24.4 -- not a known variable star
23:20:43.26 +52:38:33.1 -- not a known variable star
23:20:50.50 +57:13:03.5 -- not a known variable star
23:21:14.61 +55:23:14.2 -- not a known variable star
23:21:37.66 +55:42:58.6 -- not a known variable star
23:21:38.87 +55:10:54.8 -- not a known variable star
23:22:36.38 +57:23:00.6 -- not a known variable star
23:23:03.56 +55:52:07.8 -- not a known variable star
23:23:47.39 +54:34:22.6 -- a known variable star
23:24:57.21 +55:06:10.1 -- not a known variable star
23:25:04.78 +55:05:34.9 -- not a known variable star
23:25:10.72 +52:02:46.6 -- not a known variable star
23:25:19.25 +53:20:34.4 -- a known variable star
23:25:57.98 +53:09:48.4 -- not a known variable star
23:26:19.29 +51:13:15.1 -- not a known variable star
23:26:31.98 +54:58:42.3 -- not a known variable star
23:27:06.64 +56:40:01.5 -- a known variable star
23:27:31.99 +51:51:35.2 -- not a known variable star
23:27:35.79 +56:17:57.1 -- not a known variable star
23:28:23.02 +57:13:13.6 -- not a known variable star
23:28:27.08 +51:42:39.4 -- not a known variable star
23:28:46.89 +52:18:46.6 -- not a known variable star
23:29:28.48 +54:41:00.3 -- a known variable star
23:31:08.95 +54:16:09.0 -- not a known variable star
23:34:11.85 +56:47:43.9 -- a known variable star
23:34:15.89 +55:29:02.3 -- not a known variable star
23:34:22.94 +53:50:20.4 -- not a known variable star
23:36:48.34 +54:33:54.8 -- not a known variable star
23:37:54.66 +52:32:04.1 -- not a known variable star
23:39:32.15 +55:18:31.3 -- not a known variable star
23:41:58.54 +57:29:43.2 -- not a known variable star
23:42:50.97 +52:40:01.2 -- not a known variable star
23:47:38.58 +53:30:03.6 -- not a known variable star
23:47:55.55 +51:49:46.2 -- not a known variable star
23:51:39.01 +53:05:09.5 -- a known variable star
23:52:16.33 +54:38:46.5 -- a known variable star
23:57:19.02 +54:52:46.4 -- a known variable star
23:58:05.48 +56:28:01.3 -- a known variable star
Found 41 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
55 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 55 (excluding asteroids and hot pixels, 41 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)2461254.65887863 -observatory V36
07:25:59.27 +20:05:27.0 Mercury (0.2mag)
11:41:01.34 +01:55:17.7 Venus (-4.3mag)
05:31:33.62 +23:22:57.5 Mars (1.3mag)
08:37:27.50 +19:01:20.5 Jupiter (-1.8mag)
00:56:44.07 +03:19:08.2 Saturn (0.6mag)
04:10:58.62 +20:54:59.7 Uranus (5.8mag)
00:16:25.21 +00:15:31.3 Neptune (7.7mag)
20:28:43.59 -23:27:47.1 Pluto (14.4mag)
23:25:29.31 -02:30:12.2 Moon (-11.6mag)
-rw-r--r-- 1 apache apache 362 Aug 1 22:57 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461254.65887863:
08:37:30.31 +19:01:10.5 Io (6.0mag)
08:37:32.77 +19:00:58.4 Europa (6.3mag)
08:37:39.46 +19:00:28.2 Ganymede (5.5mag)
08:37:05.04 +19:02:52.3 Callisto (6.7mag)
08:35:08.81 +18:57:05.6 Himalia (15.7mag)
08:37:25.82 +19:01:28.4 Thebe (16.6mag)
08:34:36.76 +18:56:49.2 Elara (17.7mag)
08:41:30.66 +18:43:42.9 Pasiphae (17.9mag)
08:41:02.18 +19:10:20.3 Carme (19.0mag)
00:56:56.09 +03:19:01.4 Titan (8.4mag)
00:56:38.42 +03:19:04.5 Rhea (9.7mag)
00:56:36.04 +03:16:54.1 Iapetus (11.2mag)
00:56:47.17 +03:19:34.0 Hyperion (14.4mag)
00:56:14.42 +03:13:07.6 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 1 22:57 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461254.65887863:
18:41:11.27 -25:54:29.3 JWST
20:17:54.81 -13:13:43.3 Chandra
08:56:59.89 -50:15:57.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 1 22:57 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461254.65887863 -observatory V36
03:06:33.73 +16:50:41.5 17.7mag P/1996 R2 (Lagerkvist)
18:03:55.30 -34:39:07.2 13.9mag P/2010 H2 (Vales)
06:48:04.31 -68:41:20.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:08:08.63 +32:52:06.0 17.7mag C/2017 K2 (PANSTARRS)
03:24:49.79 +34:32:55.1 16.5mag P/2021 N1 (ZTF)
22:43:32.55 +31:46:20.0 17.3mag C/2022 E2 (ATLAS)
06:37:19.65 +26:38:30.4 16.8mag C/2022 N2 (PANSTARRS)
10:15:58.40 +28:44:38.9 16.9mag C/2022 QE78 (ATLAS)
09:24:47.56 +05:16:37.2 17.9mag C/2022 R6 (PANSTARRS)
15:11:38.09 -12:03:29.0 17.9mag P/2023 B1 (PANSTARRS)
21:18:57.06 +66:37:00.3 17.9mag C/2023 H5 (Lemmon)
15:54:30.90 -12:21:49.6 14.2mag C/2023 R1 (PANSTARRS)
08:01:09.02 +31:04:26.3 15.2mag C/2024 E1 (Wierzchos)
15:08:08.16 +15:37:11.2 17.7mag C/2024 G6 (ATLAS)
19:10:58.73 +42:39:00.3 13.7mag C/2024 J3 (ATLAS)
21:19:30.16 +48:45:53.4 17.6mag C/2024 R4 (PANSTARRS)
05:10:09.02 -13:03:39.5 15.5mag C/2024 T5 (ATLAS)
06:52:08.17 +25:12:52.0 17.9mag C/2025 J1 (Borisov)
07:28:02.45 -15:20:07.4 17.5mag C/2025 R3 (PANSTARRS)
10:24:36.34 +21:16:35.5 17.4mag C/2025 V2 (Rankin)
12:54:38.89 +02:44:23.6 17.0mag C/2025 Y1 (ATLAS)
16:06:22.09 +78:21:34.2 16.9mag C/2026 A2 (Bok)
03:04:46.78 +46:02:48.6 17.0mag C/2026 B2 (Sun-Gao)
11:41:53.09 +07:52:10.6 17.2mag A/2026 E1
21:51:18.37 -24:40:26.3 6.9mag 10P/Tempel
11:25:23.77 -03:02:09.5 16.2mag 29P/Schwassmann-Wachmann
04:31:34.17 +31:52:43.9 18.0mag 47P/Ashbrook-Jackson
10:55:17.46 +06:37:39.0 17.2mag 63P/Wild
00:54:12.94 -05:15:22.9 15.5mag 65P/Gunn
05:21:38.10 +20:45:33.2 13.7mag 78P/Gehrels
20:43:27.14 -22:48:25.4 17.9mag 84P/Giclas
02:54:16.25 +13:12:01.5 16.6mag 88P/Howell
07:40:05.21 +28:26:37.3 16.1mag 93P/Lovas
03:49:33.63 +14:31:53.0 17.8mag 112P/Urata-Niijima
05:36:21.30 +30:51:06.8 16.4mag 114P/Wiseman-Skiff
09:04:02.03 +27:38:34.0 15.0mag 123P/West-Hartley
11:31:42.68 -07:55:12.5 17.0mag 124P/Mrkos
05:27:29.07 +21:10:57.7 16.1mag 128P/Shoemaker-Holt
06:17:59.44 +19:10:14.5 17.9mag 131P/Mueller
00:04:05.47 +03:25:45.4 17.7mag 139P/Vaisala-Oterma
03:22:12.77 -19:54:58.1 14.3mag 161P/Hartley-IRAS
06:54:58.17 +37:23:18.4 15.7mag 162P/SidingSpring
16:50:17.38 +35:20:00.1 12.6mag 169P/NEAT
02:31:25.78 +09:21:06.7 17.6mag 220P/McNaught
16:38:50.02 -09:39:32.0 17.6mag 235P/LINEAR
20:26:44.51 -52:45:18.6 17.8mag 259P/Garradd
03:04:26.43 +22:33:09.2 15.4mag 260P/McNaught
06:46:58.00 +37:47:07.4 17.3mag 295P/LINEAR
15:08:45.08 +03:47:57.7 17.7mag 391P/Kowalski
08:55:20.53 +18:40:09.9 17.9mag 450P/LONEOS
08:26:43.46 +37:16:01.8 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 1 22:57 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -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
-rw-r--r-- 1 apache apache 5.7K Aug 1 22:57 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
-rw-r--r-- 1 apache apache 189K Aug 1 22:57 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:56:47.595 -41:35:10.45 AT 2026ujn 2026-07-13.05 20.3612
15:10:46.542 -37:24:26.89 AT 2026ujm 2026-07-13.05 22.857
15:01:15.315 -37:02:21.14 AT 2026ujl 2026-07-13.05 21.6824
14:52:23.223 -40:42:27.52 AT 2026ujk 2026-07-13.07 23.0058
14:59:45.613 -39:34:57.61 AT 2026ujj 2026-07-13.05 22.0092
15:00:19.929 -40:41:34.53 AT 2026uji 2026-07-13.07 22.5204
15:00:19.861 -36:24:20.89 AT 2026ujh 2026-07-13.05 22.1716
14:57:23.091 -39:39:46.60 AT 2026ujg 2026-07-13.05 23.6266
14:47:58.907 -40:16:21.10 AT 2026ujf 2026-07-13.05 23.0312
15:10:54.794 -37:44:45.52 AT 2026uje 2026-07-13.11 23.2507
19:04:42.066 -22:55:46.17 AT 2026ujd 2026-07-11.26 21.1019
19:35:18.696 -19:09:11.22 AT 2026ujc 2026-07-09.23 21.7061
19:41:34.696 -20:27:13.28 AT 2026ujb 2026-07-09.23 22.0814
19:46:25.378 -21:50:50.64 AT 2026uja 2026-07-09.23 22.4203
19:26:00.582 -18:45:15.21 AT 2026uiz 2026-07-09.25 21.6138
19:27:42.653 -19:03:28.43 AT 2026uiy 2026-07-09.25 22.6082
16:47:32.243 -26:43:45.46 AT 2026uix 2026-07-06.17 22.4211
20:04:03.181 -16:45:39.94 AT 2026uiw 2026-07-06.28 22.1634
16:59:37.183 -21:52:05.45 AT 2026uiv 2026-07-06.17 22.949
17:13:46.608 -19:49:54.77 AT 2026uiu 2026-07-06.22 21.5477
-rw-r--r-- 1 apache apache 88K Aug 1 22:57 tns_transients_list.txt
