This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH
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 05 08.4158 2461168.9158 11.25 01:33:12.81 +61:16:55.5
127.92984 -1.18362 galactic Cas Second-epoch detections are separated by 0.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:12.81 +61:16:55.5 (user input) | T | P | (position from user input) J-Ks=0.549+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:12.81 +61:16:55.5: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:12.81 +61:16:55.5: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 33 12.81 +61 16 55.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461168.9158,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260508.4158 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 11.19 01:20:42.13 +59:35:06.2
126.63359 -3.07620 galactic Cas Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:20:42.13 +59:35:06.2 (user input) | T | P | (position from user input) J-Ks=0.796+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:42.13 +59:35:06.2: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:42.13 +59:35:06.2: 13.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 20 42.13 +59 35 06.2 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,2461168.9158,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 11.02 01:36:49.01 +62:46:51.7
128.09416 0.36499 galactic Cas Second-epoch detections are separated by 1.0" and 6.1 pix
The object was found in VSX15" Gaia DR3 512426436360507392
Type: L
# Max. Min./Amp. JD0 Period
13.400 G 13.620 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:49.01 +62:46:51.7: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:49.01 +62:46:51.7: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 36 49.01 +62 46 51.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512426436360507392,2461168.9158,11.02,0.05,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 512426436360507392 20260508.4158 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 05 08.4158 2461168.9158 11.21 01:47:51.35 +61:11:12.5
129.67769 -0.94385 galactic Cas Second-epoch detections are separated by 2.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511214048684134528 | 01:47:54.00 +61:10:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.225+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:51.35 +61:11:12.5: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:51.35 +61:11:12.5: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 47 51.35 +61 11 12.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511214048684134528,2461168.9158,11.21,0.05,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 511214048684134528 20260508.4158 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 05 08.4158 2461168.9158 11.06 01:06:13.05 +59:33:45.7
124.80579 -3.25527 galactic Cas Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:13.05 +59:33:45.7 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:13.05 +59:33:45.7: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:13.05 +59:33:45.7: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 06 13.05 +59 33 45.7 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
target,2461168.9158,11.06,0.05,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
target 20260508.4158 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 05 08.4158 2461168.9158 11.12 01:33:19.85 +62:33:19.9
127.73771 0.07532 galactic Cas Second-epoch detections are separated by 1.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512315037781955200 | 01:33:17.17 +62:33:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.228+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:19.85 +62:33:19.9: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:19.85 +62:33:19.9: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 33 19.85 +62 33 19.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512315037781955200,2461168.9158,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512315037781955200 20260508.4158 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.99 02:20:39.63 +62:47:12.4
132.93150 1.66017 galactic Cas Second-epoch detections are separated by 1.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 513939639238148864 | 02:20:36.82 +62:47:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.398+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:39.63 +62:47:12.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:39.63 +62:47:12.4: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 02 20 39.63 +62 47 12.4 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 513939639238148864,2461168.9158,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 513939639238148864 20260508.4158 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 11.18 01:11:18.15 +59:35:40.9
125.44688 -3.18002 galactic Cas Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:11:18.15 +59:35:40.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:18.15 +59:35:40.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:18.15 +59:35:40.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 11 18.15 +59 35 40.9 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,2461168.9158,11.18,0.05,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
target 20260508.4158 11.18CV 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 05 08.4158 2461168.9158 10.93 01:15:23.17 +61:11:41.3
125.81369 -1.54287 galactic Cas Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510546374554030464 | 01:15:25.46 +61:11:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.305+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:23.17 +61:11:41.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:23.17 +61:11:41.3: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 15 23.17 +61 11 41.3 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 510546374554030464,2461168.9158,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510546374554030464 20260508.4158 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 11.05 01:08:39.06 +60:32:41.5
125.04815 -2.25614 galactic Cas Second-epoch detections are separated by 2.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:39.06 +60:32:41.5 (user input) | T | P | (position from user input) J-Ks=0.751+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:39.06 +60:32:41.5: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:39.06 +60:32:41.5: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 08 39.06 +60 32 41.5 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
target,2461168.9158,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 11.07 01:12:00.85 +64:42:19.1
125.12866 1.92136 galactic Cas Second-epoch detections are separated by 2.0" and 6.3 pix
The object was found in VSX 2" ZTF J011201.03+644221.2
Type: RS
# Max. Min./Amp. JD0 Period
14.762 g Y 0.263 g 2458343.85900 3.018403700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:00.85 +64:42:19.1: 11.90 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:00.85 +64:42:19.1: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 12 00.85 +64 42 19.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011201.03+644221.2,2461168.9158,11.07,0.05,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
ZTF J011201.03+644221.2 20260508.4158 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 05 08.4158 2461168.9158 10.96 01:33:01.63 +59:16:31.0
128.23058 -3.16793 galactic Cas Second-epoch detections are separated by 4.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J013303.78+591550.3 | 01:33:03.78 +59:15:50.3 (Gaia DR3) | SRS (local) | 16.088000000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:01.63 +59:16:31.0: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:01.63 +59:16:31.0: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 33 01.63 +59 16 31.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013303.78+591550.3,2461168.9158,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013303.78+591550.3 20260508.4158 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 05 08.4158 2461168.9158 11.04 01:26:24.82 +58:10:11.4
127.54410 -4.38836 galactic Cas Second-epoch detections are separated by 6.0" and 7.2 pix
The object was found in VSX18" Gaia DR3 413149018919573632
Type: ROT
# Max. Min./Amp. JD0 Period
12.570 G 12.610 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:24.82 +58:10:11.4: 12.03 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:24.82 +58:10:11.4: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 26 24.82 +58 10 11.4 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 413149018919573632,2461168.9158,11.04,0.05,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 413149018919573632 20260508.4158 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 05 08.4158 2461168.9158 10.87 01:47:54.48 +60:23:59.1
129.85477 -1.71076 galactic Cas Second-epoch detections are separated by 3.0" and 6.8 pix
The object was found in VSX 4" Gaia DR3 506654790588576000
Type: ROT
# Max. Min./Amp. JD0 Period
14.310 G 14.350 G 5.874900000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:54.48 +60:23:59.1: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:54.48 +60:23:59.1: 13.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 47 54.48 +60 23 59.1 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 506654790588576000,2461168.9158,10.87,0.05,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 506654790588576000 20260508.4158 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 05 08.4158 2461168.9158 10.97 01:24:54.85 +59:41:47.6
127.14898 -2.90081 galactic Cas Second-epoch detections are separated by 3.3" and 5.7 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 | 01:24:54.85 +59:41:47.6 (user input) | T | P | (position from user input) J-Ks=0.217+/-0.043 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:54.85 +59:41:47.6: 12.98 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:54.85 +59:41:47.6: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 24 54.85 +59 41 47.6 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,2461168.9158,10.97,0.05,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 20260508.4158 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 05 08.4158 2461168.9158 11.01 01:07:39.23 +59:59:18.0
124.96081 -2.81952 galactic Cas Second-epoch detections are separated by 2.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:39.23 +59:59:18.0 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.23 +59:59:18.0: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.23 +59:59:18.0: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 07 39.23 +59 59 18.0 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,2461168.9158,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.92 02:00:23.20 +64:54:52.3
130.15935 3.01474 galactic Cas Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:00:23.20 +64:54:52.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:23.20 +64:54:52.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:23.20 +64:54:52.3: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 02 00 23.20 +64 54 52.3 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
target,2461168.9158,10.92,0.05,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
target 20260508.4158 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 05 08.4158 2461168.9158 10.90 01:29:02.66 +58:46:10.3
127.80088 -3.74625 galactic Cas Second-epoch detections are separated by 4.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J012906.85+584639.3 | 01:29:06.84 +58:46:39.2 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:02.66 +58:46:10.3: 12.74 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:02.66 +58:46:10.3: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 29 02.66 +58 46 10.3 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
ASASSN-V J012906.85+584639.3,2461168.9158,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J012906.85+584639.3 20260508.4158 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.84 01:54:45.26 +57:45:51.6
131.31924 -4.07266 galactic Per Second-epoch detections are separated by 2.7" and 6.7 pix
The object was found in VSX23" Gaia DR3 506102938826140544
Type: ROT
# Max. Min./Amp. JD0 Period
13.250 G 13.270 G 11.769600000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:45.26 +57:45:51.6: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:45.26 +57:45:51.6: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 54 45.26 +57 45 51.6 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 506102938826140544,2461168.9158,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506102938826140544 20260508.4158 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.79 02:07:25.22 +57:54:57.6
132.90641 -3.47674 galactic Per Second-epoch detections are separated by 1.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506730034109607680 | 02:07:24.66 +57:55:23.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:25.22 +57:54:57.6: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:25.22 +57:54:57.6: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 02 07 25.22 +57 54 57.6 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 506730034109607680,2461168.9158,10.79,0.05,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 506730034109607680 20260508.4158 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 05 08.4158 2461168.9158 10.85 01:28:32.99 +61:12:18.8
127.38709 -1.34509 galactic Cas Second-epoch detections are separated by 3.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | PQ Cas | 01:28:36.18 +61:12:07.5 (Gaia DR3) | SR (local) | 2458436.69130 (local) | Gaia3var=VARIABLE SpType: S 1975AbaOB..47....3D [D75b] Star 4
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:32.99 +61:12:18.8: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:32.99 +61:12:18.8: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 28 32.99 +61 12 18.8 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
PQ Cas,2461168.9158,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PQ Cas 20260508.4158 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.71 01:43:26.09 +58:38:22.4
129.66749 -3.55054 galactic Cas Second-epoch detections are separated by 2.4" and 6.7 pix
The object was found in VSX20" Gaia DR3 506084487648397824
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:26.09 +58:38:22.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:26.09 +58:38:22.4: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 43 26.09 +58 38 22.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506084487648397824,2461168.9158,10.71,0.05,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
Gaia DR3 506084487648397824 20260508.4158 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 05 08.4158 2461168.9158 10.85 01:13:44.71 +57:24:50.8
125.94504 -5.32707 galactic Cas Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:13:44.71 +57:24:50.8 (user input) | T | P | (position from user input) J-Ks=0.655+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:44.71 +57:24:50.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:44.71 +57:24:50.8: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 13 44.71 +57 24 50.8 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461168.9158,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.74 01:09:22.07 +64:35:17.1
124.85478 1.78330 galactic Cas Second-epoch detections are separated by 3.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:09:22.07 +64:35:17.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.07 +64:35:17.1: 12.76 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.07 +64:35:17.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 09 22.07 +64 35 17.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461168.9158,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.73 01:07:35.13 +57:33:10.4
125.10565 -5.25069 galactic Cas Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:35.13 +57:33:10.4 (user input) | T | P | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.856+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:35.13 +57:33:10.4: 12.16 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:35.13 +57:33:10.4: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 07 35.13 +57 33 10.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461168.9158,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.85 01:32:05.66 +61:59:26.0
127.68580 -0.50535 galactic Cas Second-epoch detections are separated by 2.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510798197068398848 | 01:32:04.51 +61:59:00.7 (Gaia DR3) | DSCT/GDOR (local) | A (local) | Gaia3var=VARIABLE SpType: F5 1960IzKry..24..160B [B60] +61 281 J-Ks=0.127+/-0.036 (A)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:05.66 +61:59:26.0: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:05.66 +61:59:26.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 32 05.66 +61 59 26.0 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 510798197068398848,2461168.9158,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510798197068398848 20260508.4158 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.79 01:52:47.83 +58:10:25.5
130.96836 -3.73737 galactic Cas Second-epoch detections are separated by 1.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J028.1896+58.1775 | 01:52:46.32 +58:10:45.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.086+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:47.83 +58:10:25.5: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:47.83 +58:10:25.5: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 52 47.83 +58 10 25.5 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
ATO J028.1896+58.1775,2461168.9158,10.79,0.05,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
ATO J028.1896+58.1775 20260508.4158 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 05 08.4158 2461168.9158 10.59 01:37:09.79 +58:51:05.8
128.82703 -3.49578 galactic Cas Second-epoch detections are separated by 1.6" and 6.5 pix
The object was found in VSX15" Gaia DR3 509131131290597376
Type: ROT
# Max. Min./Amp. JD0 Period
16.600 G 16.660 G 1.529270000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:09.79 +58:51:05.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:09.79 +58:51:05.8: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 37 09.79 +58 51 05.8 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509131131290597376,2461168.9158,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 509131131290597376 20260508.4158 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.66 01:09:09.17 +61:37:28.2
125.03548 -1.17487 galactic Cas Second-epoch detections are separated by 1.7" and 5.9 pix
The object was found in VSX 2" Gaia DR3 522536136541501952
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.570 G 13.610 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:09.17 +61:37:28.2: 12.93 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:09.17 +61:37:28.2: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 09 09.17 +61 37 28.2 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522536136541501952,2461168.9158,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522536136541501952 20260508.4158 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.74 01:17:15.30 +58:35:37.9
126.29872 -4.10902 galactic Cas Second-epoch detections are separated by 3.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J019.3185+58.5958 | 01:17:17.58 +58:36:18.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1960IzKry..24..160B [B60] +58 130
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:15.30 +58:35:37.9: 12.66 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:15.30 +58:35:37.9: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 17 15.30 +58 35 37.9 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.3185+58.5958,2461168.9158,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.3185+58.5958 20260508.4158 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.34 01:04:09.39 +63:14:43.6
124.36275 0.40904 galactic Cas Second-epoch detections are separated by 5.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:04:09.39 +63:14:43.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:09.39 +63:14:43.6: 10.88 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:09.39 +63:14:43.6: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 04 09.39 +63 14 43.6 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461168.9158,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.44 01:31:22.94 +59:33:43.3
127.97841 -2.91777 galactic Cas Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J022.8294+59.5638 | 01:31:22.94 +59:33:43.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.833+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:22.94 +59:33:43.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:22.94 +59:33:43.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 31 22.94 +59 33 43.3 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.8294+59.5638,2461168.9158,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.8294+59.5638 20260508.4158 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.09 01:11:15.92 +61:08:30.7
125.32299 -1.63780 galactic Cas Second-epoch detections are separated by 1.1" and 6.3 pix
The object was found in VSX14" ZTF J011114.91+610818.6
Type: RS
# Max. Min./Amp. JD0 Period
13.623 g Y 0.083 g 2458358.91940 0.779401400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:15.92 +61:08:30.7: 12.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:15.92 +61:08:30.7: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 11 15.92 +61 08 30.7 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011114.91+610818.6,2461168.9158,10.09,0.05,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
ZTF J011114.91+610818.6 20260508.4158 10.09CV 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 05 08.4158 2461168.9158 9.93 01:25:26.50 +60:57:44.8
127.04822 -1.63725 galactic Cas Second-epoch detections are separated by 0.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510670688089089920 | 01:25:28.22 +60:57:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +60 212 J-Ks=0.332+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:26.50 +60:57:44.8: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:26.50 +60:57:44.8: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 25 26.50 +60 57 44.8 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510670688089089920,2461168.9158,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510670688089089920 20260508.4158 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 9.82 01:23:31.41 +58:41:47.7
127.09938 -3.91530 galactic Cas Second-epoch detections are separated by 0.7" and 6.3 pix
The object was found in VSX22" Gaia DR3 413949673852809088
Type: ROT
# Max. Min./Amp. JD0 Period
16.410 G 16.550 G 1.041480000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:31.41 +58:41:47.7: 12.06 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:31.41 +58:41:47.7: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 23 31.41 +58 41 47.7 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413949673852809088,2461168.9158,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413949673852809088 20260508.4158 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 9.71 01:20:24.26 +59:10:25.0
126.64239 -3.48929 galactic Cas Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J020.1204+59.1623 | 01:20:25.01 +59:10:05.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.296+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:24.26 +59:10:25.0: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:24.26 +59:10:25.0: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 20 24.26 +59 10 25.0 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J020.1204+59.1623,2461168.9158,9.71,0.05,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 J020.1204+59.1623 20260508.4158 9.71CV 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 05 08.4158 2461168.9158 9.65 01:15:16.74 +57:28:04.8
126.14659 -5.25486 galactic Cas Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413443898501160704 | 01:15:18.56 +57:27:47.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.238+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:16.74 +57:28:04.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:16.74 +57:28:04.8: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 15 16.74 +57 28 04.8 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413443898501160704,2461168.9158,9.65,0.05,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 413443898501160704 20260508.4158 9.65CV 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 05 08.4158 2461168.9158 9.39 01:52:08.93 +58:27:41.2
130.81779 -3.47769 galactic Cas Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506205674446445952 | 01:52:09.03 +58:27:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:08.93 +58:27:41.2: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:08.93 +58:27:41.2: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 52 08.93 +58 27 41.2 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 506205674446445952,2461168.9158,9.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506205674446445952 20260508.4158 9.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 8.21 01:47:13.08 +57:44:19.0
130.34399 -4.32818 galactic Cas Second-epoch detections are separated by 1.5" and 6.4 pix
The object was found in VSX 4" Gaia DR3 505962471920178944
Type: VAR
# Max. Min./Amp. JD0 Period
13.440 G 13.470 G 0.024984900000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:13.08 +57:44:19.0: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:13.08 +57:44:19.0: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.71 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 47 13.08 +57 44 19.0 8.2 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 505962471920178944,2461168.9158,8.21,0.05,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 505962471920178944 20260508.4158 8.21CV 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 05 08.4158 2461168.9158 7.49 01:35:37.81 +61:16:52.0
128.21634 -1.13640 galactic Cas Second-epoch detections are separated by 6.6" and 5.3 pix
The object was found in VSX11" Gaia DR3 509978579881384704
Type: E
# Max. Min./Amp. JD0 Period
12.390 G 12.580 G 1.177150000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:37.81 +61:16:52.0: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:37.81 +61:16:52.0: 10.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 35 37.81 +61 16 52.0 7.5 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 509978579881384704,2461168.9158,7.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509978579881384704 20260508.4158 7.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 9.20 01:28:00.35 +61:19:59.2
127.30414 -1.22782 galactic Cas Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510703497331624576 | 01:28:01.22 +61:19:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S BD+60 240 J-Ks=0.169+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:00.35 +61:19:59.2: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:00.35 +61:19:59.2: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 28 00.35 +61 19 59.2 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510703497331624576,2461168.9158,9.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510703497331624576 20260508.4158 9.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.61 01:46:38.35 +60:07:34.1
129.75982 -2.01178 galactic Cas Second-epoch detections are separated by 2.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.6591+60.1406 | 01:46:39.63 +60:07:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.35 +60:07:34.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.35 +60:07:34.1: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 46 38.35 +60 07 34.1 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
ATO J026.6591+60.1406,2461168.9158,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.6591+60.1406 20260508.4158 10.61CV 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 05 08.4158 2461168.9158 10.77 02:01:03.48 +64:43:34.6
130.27830 2.85218 galactic Cas Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:01:03.48 +64:43:34.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:03.48 +64:43:34.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:03.48 +64:43:34.6: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 02 01 03.48 +64 43 34.6 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
target,2461168.9158,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260508.4158 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.68 01:51:09.31 +64:52:47.1
129.21800 2.73935 galactic Cas Second-epoch detections are separated by 2.2" and 5.9 pix
The object was found in VSX 2" Gaia DR3 518229967963921664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:09.31 +64:52:47.1: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.31 +64:52:47.1: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 51 09.31 +64 52 47.1 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
Gaia DR3 518229967963921664,2461168.9158,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518229967963921664 20260508.4158 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.76 02:02:50.53 +60:13:59.2
131.68851 -1.41903 galactic Cas Second-epoch detections are separated by 1.2" and 6.5 pix
The object was found in VSX21" Gaia DR3 507950766893076736
Type: E
# Max. Min./Amp. JD0 Period
18.720 G 19.250 G 0.254094000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:50.53 +60:13:59.2: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:50.53 +60:13:59.2: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 02 02 50.53 +60 13 59.2 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 507950766893076736,2461168.9158,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507950766893076736 20260508.4158 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.70 01:26:35.73 +57:57:38.8
127.59653 -4.59220 galactic Cas Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.6500+57.9729 | 01:26:33.58 +57:57:55.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.441+/-0.037 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:35.73 +57:57:38.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:35.73 +57:57:38.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 26 35.73 +57 57 38.8 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.6500+57.9729,2461168.9158,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.6500+57.9729 20260508.4158 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.85 01:18:48.49 +64:12:26.3
125.90450 1.49364 galactic Cas Second-epoch detections are separated by 0.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:48.49 +64:12:26.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:48.49 +64:12:26.3: 11.87 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:48.49 +64:12:26.3: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 18 48.49 +64 12 26.3 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
target,2461168.9158,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.76 01:32:40.21 +61:07:38.8
127.89005 -1.34675 galactic Cas Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:32:40.21 +61:07:38.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:40.21 +61:07:38.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:40.21 +61:07:38.8: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 32 40.21 +61 07 38.8 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461168.9158,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.82 01:11:56.35 +58:41:02.1
125.60002 -4.08159 galactic Cas Second-epoch detections are separated by 3.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.9933+58.6776 | 01:11:56.35 +58:41:02.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:56.35 +58:41:02.1: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:56.35 +58:41:02.1: 13.87 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 05 08.4158* 01 11 56.35 +58 41 02.1 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
ATO J017.9933+58.6776,2461168.9158,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.9933+58.6776 20260508.4158 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.93 01:38:05.79 +61:04:14.5
128.54596 -1.29145 galactic Cas Second-epoch detections are separated by 1.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:38:05.79 +61:04:14.5 (user input) | T | P | (position from user input) J-Ks=0.901+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.79 +61:04:14.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:05.79 +61:04:14.5: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 38 05.79 +61 04 14.5 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
target,2461168.9158,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.83 01:14:58.38 +60:30:24.8
125.82695 -2.23250 galactic Cas Second-epoch detections are separated by 2.9" and 6.6 pix
The object was found in VSX 4" Mis V1361
Type: EA
# Max. Min./Amp. JD0 Period
13.551 r Y 0.490 r 2458282.97450 1.603348400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:58.38 +60:30:24.8: 12.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:58.38 +60:30:24.8: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 14 58.38 +60 30 24.8 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1361,2461168.9158,10.83,0.05,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
Mis V1361 20260508.4158 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 05 08.4158 2461168.9158 10.86 01:06:55.35 +59:18:56.6
124.90996 -3.49654 galactic Cas Second-epoch detections are separated by 3.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.35 +59:18:56.6 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.35 +59:18:56.6: 13.07 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.35 +59:18:56.6: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 06 55.35 +59 18 56.6 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
target,2461168.9158,10.86,0.05,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
target 20260508.4158 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 05 08.4158 2461168.9158 10.96 01:31:48.42 +64:22:26.5
127.28066 1.84367 galactic Cas Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.42 +64:22:26.5 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.42 +64:22:26.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.42 +64:22:26.5: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 31 48.42 +64 22 26.5 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
target,2461168.9158,10.96,0.05,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
target 20260508.4158 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 05 08.4158 2461168.9158 10.95 02:16:02.26 +60:36:56.0
133.12968 -0.57023 galactic Cas Second-epoch detections are separated by 1.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:16:02.26 +60:36:56.0 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:02.26 +60:36:56.0: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:02.26 +60:36:56.0: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 02 16 02.26 +60 36 56.0 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
target,2461168.9158,10.95,0.05,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
target 20260508.4158 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 05 08.4158 2461168.9158 10.88 01:13:38.83 +58:10:50.9
125.86532 -4.56439 galactic Cas Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J018.4234+58.1762 | 01:13:41.63 +58:10:34.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.593+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:38.83 +58:10:50.9: 13.01 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:38.83 +58:10:50.9: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 13 38.83 +58 10 50.9 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 J018.4234+58.1762,2461168.9158,10.88,0.05,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
ATO J018.4234+58.1762 20260508.4158 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 05 08.4158 2461168.9158 10.95 01:43:03.24 +58:57:14.1
129.55615 -3.25238 galactic Cas Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.7767+58.9545 | 01:43:03.24 +58:57:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.236+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:03.24 +58:57:14.1: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:03.24 +58:57:14.1: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 43 03.24 +58 57 14.1 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 J025.7767+58.9545,2461168.9158,10.95,0.05,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
ATO J025.7767+58.9545 20260508.4158 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 05 08.4158 2461168.9158 11.04 01:26:05.40 +59:01:14.8
127.38707 -3.55090 galactic Cas Second-epoch detections are separated by 3.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.5231+59.0209 | 01:26:05.40 +59:01:14.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.40 +59:01:14.8: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.40 +59:01:14.8: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 26 05.40 +59 01 14.8 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 J021.5231+59.0209,2461168.9158,11.04,0.05,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 J021.5231+59.0209 20260508.4158 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 05 08.4158 2461168.9158 11.18 01:42:17.42 +63:24:22.4
128.58671 1.09416 galactic Cas Second-epoch detections are separated by 3.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512081945620708864 | 01:42:22.23 +63:24:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.949+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:17.42 +63:24:22.4: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:17.42 +63:24:22.4: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 42 17.42 +63 24 22.4 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 512081945620708864,2461168.9158,11.18,0.05,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 512081945620708864 20260508.4158 11.18CV 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 05 08.4158 2461168.9158 11.07 01:54:30.39 +59:06:33.9
130.96063 -2.77568 galactic Cas Second-epoch detections are separated by 2.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J028.5927+59.1125 | 01:54:25.94 +59:06:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.337+/-0.133 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:30.39 +59:06:33.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:30.39 +59:06:33.9: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 54 30.39 +59 06 33.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J028.5927+59.1125,2461168.9158,11.07,0.05,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
ATO J028.5927+59.1125 20260508.4158 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 05 08.4158 2461168.9158 11.11 01:48:35.05 +58:41:32.4
130.31203 -3.35816 galactic Cas Second-epoch detections are separated by 4.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J027.1136+58.6801 | 01:48:31.31 +58:41:04.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:35.05 +58:41:32.4: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:35.05 +58:41:32.4: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 48 35.05 +58 41 32.4 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 J027.1136+58.6801,2461168.9158,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J027.1136+58.6801 20260508.4158 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 11.16 01:44:15.59 +61:53:38.5
129.11021 -0.34244 galactic Cas Second-epoch detections are separated by 2.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:44:15.59 +61:53:38.5 (user input) | T | P | (position from user input) J-Ks=0.208+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:15.59 +61:53:38.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:15.59 +61:53:38.5: 14.03 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 44 15.59 +61 53 38.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461168.9158,11.16,0.05,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 20260508.4158 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 05 08.4158 2461168.9158 11.21 01:26:28.43 +59:41:37.2
127.34462 -2.87757 galactic Cas Second-epoch detections are separated by 4.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.6536+59.6928 | 01:26:31.85 +59:41:21.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:28.43 +59:41:37.2: 12.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:28.43 +59:41:37.2: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 26 28.43 +59 41 37.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.6536+59.6928,2461168.9158,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.6536+59.6928 20260508.4158 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 05 08.4158 2461168.9158 11.38 01:37:39.85 +60:37:33.1
128.57388 -1.73851 galactic Cas Second-epoch detections are separated by 5.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509897662695283200 | 01:37:42.91 +60:38:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1955ApJS....2..123F LF 5 +60 125 J-Ks=0.766+/-0.043 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:39.85 +60:37:33.1: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:39.85 +60:37:33.1: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 05 08.4158* 01 37 39.85 +60 37 33.1 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509897662695283200,2461168.9158,11.38,0.05,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 509897662695283200 20260508.4158 11.38CV 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 05 08.4158 2461168.9158 11.33 01:49:09.98 +60:03:40.1
130.08162 -2.00681 galactic Cas Second-epoch detections are separated by 2.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506634312183863424 | 01:49:13.50 +60:04:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0III 1932MeUpp..55....1S BD+59 327 J-Ks=0.435+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:09.98 +60:03:40.1: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:09.98 +60:03:40.1: 14.37 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 49 09.98 +60 03 40.1 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506634312183863424,2461168.9158,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 506634312183863424 20260508.4158 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 11.57 02:14:18.46 +62:21:00.6
132.38230 1.00867 galactic Cas Second-epoch detections are separated by 1.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 514571720976048896 | 02:14:13.89 +62:20:56.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.429+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:18.46 +62:21:00.6: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:18.46 +62:21:00.6: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 02 14 18.46 +62 21 00.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 514571720976048896,2461168.9158,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 514571720976048896 20260508.4158 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 9.40 02:18:22.35 +58:47:11.2
134.00368 -2.20391 galactic Per Second-epoch detections are separated by 0.4" and 6.5 pix
The object was found in VSX 4" NSVS J0218236+584716
Type: SR
# Max. Min./Amp. JD0 Period
12.694 r Y 0.560 r 2458351.79460 241.646383300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:22.35 +58:47:11.2: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:22.35 +58:47:11.2: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 02 18 22.35 +58 47 11.2 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0218236+584716,2461168.9158,9.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0218236+584716 20260508.4158 9.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 08.4158 2461168.9158 10.98 01:33:44.34 +60:46:19.4
128.07550 -1.67655 galactic Cas Second-epoch detections are separated by 5.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:44.34 +60:46:19.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:44.34 +60:46:19.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.34 +60:46:19.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 08.4158* 01 33 44.34 +60 46 19.4 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
target,2461168.9158,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260508.4158 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461168.91609067 08.05.2026 09:59:00.234 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 25306
Objects passed selection criteria: 25149
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: 17489.8
Average stars matched: 16090.2 (91.9982 %)
Memory usage VmPeak: 128284 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri May 8 05:03:04 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: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461168.91609067 08.05.2026 09:59:00.234 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 212
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
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: 90 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 185718
Objects passed selection criteria: 185239
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 136339
Average stars matched: 125216 (91.8419 %)
Memory usage VmPeak: 2000192 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri May 8 05:08:47 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.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: 2461168.91551087
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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:43:02.195 +61:56:58.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:02.195 +61:56:58.31
Angular distance between the image centers 0.0746 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:43:04.297 +61:57:32.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:04.297 +61:57:32.60
Angular distance between the image centers 0.0744 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 01:43:02.195 +61:56:58.31
Second-epoch second image center 01:43:04.297 +61:57:32.60
Angular distance between the image centers 0.01038 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.VrS85hXlJ9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.fwpEWv6koQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits &> /tmp/tmp.VZ8GPw1aJY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits &> /tmp/tmp.96fNfld64B
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 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 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 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): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929150
a=0.000000 b=1.000000 c=22.929150
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 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 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 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): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.8)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 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 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 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): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
14.3 mag. fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
14.3 mag. fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.4 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.VrS85hXlJ9 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 266 matched stars entering correct_measured_positions(), 9996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 337 matched stars entering correct_measured_positions(), 10041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.88"
Excluding outliers - 331 stars left (next iteration limit 292)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fwpEWv6koQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VZ8GPw1aJY (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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1134, passed=14407
Got 14407 stars (including 13263 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 14407 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.2)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 14074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.2)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 14077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 14077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.96fNfld64B (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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1154, passed=14409
Got 14409 stars (including 13250 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat
util/solve_plate_with_UCAC5 got 14409 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.2)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 14017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.2)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 14017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 14017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 969 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:11.33 +58:01:02.8: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:34.86 +59:08:13.5: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:34.86 +59:08:13.5: 11.49 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:11.33 +58:01:02.8: 10.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.58 +/- 0.00
Forced photometry reference-image weighted average: 11.49 +/- 0.01
Forced photometry filter REJECTED candidate at 02:09:11.33 +58:01:02.8: ref_mag=10.58 +/- 0.00 new_mean_mag=10.8489 delta=-0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:00:34.86 +59:08:13.5: ref_mag=11.49 +/- 0.01 new_mean_mag=11.7510 delta=-0.26 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 51603_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 51603_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51605_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 51605_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52671_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 52671_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:19:46.42 +58:12:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 08339_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:20:32.53 +62:32:01.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:43:02.195 +61:56:58.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:02.195 +61:56:58.31
Angular distance between the image centers 0.0746 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:43:04.297 +61:57:32.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:04.297 +61:57:32.60
Angular distance between the image centers 0.0744 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 01:43:02.195 +61:56:58.31
Second-epoch second image center 01:43:04.297 +61:57:32.60
Angular distance between the image centers 0.01038 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.5n9d6bYbAB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.ClFPlF7aEK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits &> /tmp/tmp.eTd2Cx5Udu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits &> /tmp/tmp.QOA4VWfi0p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 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 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 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): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.035150
a=0.000000 b=1.000000 c=20.035150
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.76
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 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 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 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): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=4.4)
Read 218998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9707 to 45.8168 deg, Dec +55.3262 to +67.4140 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 6.9707 to 45.8168 deg, Dec 55.3262 to 67.4140 deg
Loaded 26295 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): 10859 out of 16691 total matches.
Matched with Tycho-2 16691 out of 218998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 196 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.3 pix fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
2.2 pix fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
12.8 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
12.7 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
11.7 mag. fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
11.7 mag. fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
All-image limiting magnitude estimate: 11.7 (SNR ) 11.2 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5n9d6bYbAB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=35398, passed=222522
Got 222522 stars (including 186791 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 222522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 275 matched stars entering correct_measured_positions(), 212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 264 matched stars entering correct_measured_positions(), 49591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 434 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 49636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
Accuracy estimation diagnostic: 344 matched stars entering correct_measured_positions(), 64908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.78"
Excluding outliers - 344 stars left (next iteration limit 290)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ClFPlF7aEK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=35098, passed=218974
Got 218974 stars (including 183551 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 218974 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eTd2Cx5Udu (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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=10085, passed=108908
Got 108908 stars (including 98702 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 108908 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 106811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 106811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 106811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QOA4VWfi0p (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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=10246, passed=110505
Got 110505 stars (including 100135 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat
util/solve_plate_with_UCAC5 got 110505 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 107934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 107936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 107935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-58-10_20.00sec_-4.90C_LIGHT_0426.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.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_2026-05-08_CI_Cas-03-Q2b1x1_050029_TTUQ2b1x1_731423_Mn2iHJBH/wcs_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427.fits
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:42.13 +59:35:06.2: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:49.01 +62:46:51.7: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:13.05 +59:33:45.7: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:12.81 +61:16:55.5: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:39.63 +62:47:12.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:19.85 +62:33:19.9: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:18.15 +59:35:40.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:51.35 +61:11:12.5: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:42.13 +59:35:06.2: 13.89 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:18.15 +59:35:40.9: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:51.35 +61:11:12.5: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:39.06 +60:32:41.5: 13.27 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Forced photometry filter KEPT candidate at 01:20:42.13 +59:35:06.2: ref_mag=13.89 +/- 0.04 new_mean_mag=11.1576 delta=2.73 (need > 0.90)
Forced photometry filter KEPT candidate at 01:11:18.15 +59:35:40.9: ref_mag=13.84 +/- 0.05 new_mean_mag=11.1488 delta=2.70 (need > 0.90)
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Forced photometry filter KEPT candidate at 01:47:51.35 +61:11:12.5: ref_mag=13.86 +/- 0.05 new_mean_mag=11.2116 delta=2.65 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:12.81 +61:16:55.5: 14.11 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:19.85 +62:33:19.9: 13.74 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:13.05 +59:33:45.7: 13.58 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:39.63 +62:47:12.4: 13.50 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:23.17 +61:11:41.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:49.01 +62:46:51.7: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.06
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Forced photometry filter KEPT candidate at 01:33:12.81 +61:16:55.5: ref_mag=14.11 +/- 0.06 new_mean_mag=11.2379 delta=2.87 (need > 0.90)
Forced photometry filter KEPT candidate at 01:06:13.05 +59:33:45.7: ref_mag=13.58 +/- 0.04 new_mean_mag=11.0591 delta=2.53 (need > 0.90)
Forced photometry filter KEPT candidate at 01:33:19.85 +62:33:19.9: ref_mag=13.74 +/- 0.04 new_mean_mag=11.1220 delta=2.61 (need > 0.90)
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Forced photometry filter KEPT candidate at 02:20:39.63 +62:47:12.4: ref_mag=13.50 +/- 0.04 new_mean_mag=10.9911 delta=2.51 (need > 0.90)
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Forced photometry filter KEPT candidate at 01:36:49.01 +62:46:51.7: ref_mag=13.66 +/- 0.04 new_mean_mag=10.9543 delta=2.71 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:39.06 +60:32:41.5: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry filter KEPT candidate at 01:08:39.06 +60:32:41.5: ref_mag=13.91 +/- 0.05 new_mean_mag=11.0541 delta=2.86 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:23.17 +61:11:41.3: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 01:15:23.17 +61:11:41.3: ref_mag=13.43 +/- 0.03 new_mean_mag=10.9189 delta=2.51 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:00.85 +64:42:19.1: 11.90 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:00.85 +64:42:19.1: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Forced photometry filter KEPT candidate at 01:12:00.85 +64:42:19.1: ref_mag=13.44 +/- 0.04 new_mean_mag=11.0758 delta=2.37 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:01.63 +59:16:31.0: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:01.63 +59:16:31.0: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Forced photometry filter KEPT candidate at 01:33:01.63 +59:16:31.0: ref_mag=13.87 +/- 0.05 new_mean_mag=10.9556 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:24.82 +58:10:11.4: 12.03 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:24.82 +58:10:11.4: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 01:26:24.82 +58:10:11.4: ref_mag=13.48 +/- 0.03 new_mean_mag=11.0279 delta=2.45 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:54.48 +60:23:59.1: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:54.48 +60:23:59.1: 13.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 01:47:54.48 +60:23:59.1: ref_mag=13.31 +/- 0.02 new_mean_mag=10.8678 delta=2.45 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:54.85 +59:41:47.6: 12.98 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.23 +59:59:18.0: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:54.85 +59:41:47.6: 13.96 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:23.20 +64:54:52.3: 13.28 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry filter KEPT candidate at 01:24:54.85 +59:41:47.6: ref_mag=13.93 +/- 0.05 new_mean_mag=10.9720 delta=2.95 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:02.66 +58:46:10.3: 12.74 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:45.26 +57:45:51.6: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.23 +59:59:18.0: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 01:07:39.23 +59:59:18.0: ref_mag=13.74 +/- 0.04 new_mean_mag=11.0007 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:23.20 +64:54:52.3: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter KEPT candidate at 02:00:23.20 +64:54:52.3: ref_mag=13.60 +/- 0.04 new_mean_mag=10.9190 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:45.26 +57:45:51.6: 13.68 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:02.66 +58:46:10.3: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Forced photometry filter KEPT candidate at 01:54:45.26 +57:45:51.6: ref_mag=13.68 +/- 0.05 new_mean_mag=10.8356 delta=2.84 (need > 0.90)
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Forced photometry filter KEPT candidate at 01:29:02.66 +58:46:10.3: ref_mag=13.75 +/- 0.05 new_mean_mag=10.9013 delta=2.85 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:25.22 +57:54:57.6: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:25.22 +57:54:57.6: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter KEPT candidate at 02:07:25.22 +57:54:57.6: ref_mag=13.48 +/- 0.04 new_mean_mag=10.7948 delta=2.68 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:32.99 +61:12:18.8: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:32.99 +61:12:18.8: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Forced photometry filter KEPT candidate at 01:28:32.99 +61:12:18.8: ref_mag=13.79 +/- 0.05 new_mean_mag=10.8511 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:26.09 +58:38:22.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:26.09 +58:38:22.4: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter KEPT candidate at 01:43:26.09 +58:38:22.4: ref_mag=13.60 +/- 0.04 new_mean_mag=10.6957 delta=2.91 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:44.71 +57:24:50.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:44.71 +57:24:50.8: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 01:13:44.71 +57:24:50.8: ref_mag=13.48 +/- 0.03 new_mean_mag=10.8463 delta=2.63 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.07 +64:35:17.1: 12.76 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.07 +64:35:17.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Forced photometry filter KEPT candidate at 01:09:22.07 +64:35:17.1: ref_mag=13.63 +/- 0.04 new_mean_mag=10.7332 delta=2.89 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:35.13 +57:33:10.4: 12.16 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:35.13 +57:33:10.4: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 01:07:35.13 +57:33:10.4: ref_mag=13.45 +/- 0.03 new_mean_mag=10.7302 delta=2.72 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:05.66 +61:59:26.0: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:05.66 +61:59:26.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 01:32:05.66 +61:59:26.0: ref_mag=13.45 +/- 0.03 new_mean_mag=10.8356 delta=2.62 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:47.83 +58:10:25.5: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:47.83 +58:10:25.5: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Forced photometry filter KEPT candidate at 01:52:47.83 +58:10:25.5: ref_mag=13.24 +/- 0.03 new_mean_mag=10.7703 delta=2.47 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:09.79 +58:51:05.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:09.79 +58:51:05.8: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 01:37:09.79 +58:51:05.8: ref_mag=13.33 +/- 0.03 new_mean_mag=10.5779 delta=2.75 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:09.17 +61:37:28.2: 12.93 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:09.17 +61:37:28.2: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter KEPT candidate at 01:09:09.17 +61:37:28.2: ref_mag=13.31 +/- 0.03 new_mean_mag=10.6547 delta=2.66 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:15.30 +58:35:37.9: 12.66 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:15.30 +58:35:37.9: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Forced photometry filter KEPT candidate at 01:17:15.30 +58:35:37.9: ref_mag=13.46 +/- 0.04 new_mean_mag=10.7356 delta=2.72 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:09.39 +63:14:43.6: 10.88 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:10.38 +60:37:30.4: 7.59 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:09.39 +63:14:43.6: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Forced photometry filter KEPT candidate at 01:04:09.39 +63:14:43.6: ref_mag=12.53 +/- 0.02 new_mean_mag=10.2472 delta=2.28 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:10.38 +60:37:30.4: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 7.86 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:10.38 +60:37:30.4: ref_mag=7.86 +/- 0.01 new_mean_mag=10.5131 delta=-2.65 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:22.94 +59:33:43.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:22.94 +59:33:43.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Forced photometry filter KEPT candidate at 01:31:22.94 +59:33:43.3: ref_mag=13.22 +/- 0.03 new_mean_mag=10.4338 delta=2.79 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:15.92 +61:08:30.7: 12.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:15.92 +61:08:30.7: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Forced photometry filter KEPT candidate at 01:11:15.92 +61:08:30.7: ref_mag=12.70 +/- 0.02 new_mean_mag=10.0875 delta=2.61 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:26.50 +60:57:44.8: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:26.50 +60:57:44.8: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 01:25:26.50 +60:57:44.8: ref_mag=12.68 +/- 0.01 new_mean_mag=9.9309 delta=2.75 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:31.41 +58:41:47.7: 12.06 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:16.74 +57:28:04.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:24.26 +59:10:25.0: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:16.74 +57:28:04.8: 12.40 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:31.41 +58:41:47.7: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 01:23:31.41 +58:41:47.7: ref_mag=12.52 +/- 0.01 new_mean_mag=9.8126 delta=2.70 (need > 0.90)
Forced photometry filter KEPT candidate at 01:15:16.74 +57:28:04.8: ref_mag=12.40 +/- 0.01 new_mean_mag=9.6499 delta=2.75 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:24.26 +59:10:25.0: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 01:20:24.26 +59:10:25.0: ref_mag=12.33 +/- 0.01 new_mean_mag=9.7099 delta=2.62 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:08.93 +58:27:41.2: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:08.93 +58:27:41.2: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 01:52:08.93 +58:27:41.2: ref_mag=11.92 +/- 0.01 new_mean_mag=9.3755 delta=2.54 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:13.08 +57:44:19.0: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:13.08 +57:44:19.0: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.71 +/- 0.00
Forced photometry filter KEPT candidate at 01:47:13.08 +57:44:19.0: ref_mag=10.71 +/- 0.00 new_mean_mag=8.1939 delta=2.52 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:37.81 +61:16:52.0: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:37.81 +61:16:52.0: 10.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.06 +/- 0.00
Forced photometry filter KEPT candidate at 01:35:37.81 +61:16:52.0: ref_mag=10.06 +/- 0.00 new_mean_mag=7.4073 delta=2.66 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:00.35 +61:19:59.2: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:00.35 +61:19:59.2: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Forced photometry filter KEPT candidate at 01:28:00.35 +61:19:59.2: ref_mag=11.80 +/- 0.01 new_mean_mag=9.1959 delta=2.60 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.35 +60:07:34.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.35 +60:07:34.1: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Forced photometry filter KEPT candidate at 01:46:38.35 +60:07:34.1: ref_mag=13.39 +/- 0.04 new_mean_mag=10.5981 delta=2.79 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:03.48 +64:43:34.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:03.48 +64:43:34.6: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.05
Forced photometry filter KEPT candidate at 02:01:03.48 +64:43:34.6: ref_mag=13.70 +/- 0.05 new_mean_mag=10.7419 delta=2.96 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:09.31 +64:52:47.1: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.31 +64:52:47.1: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Forced photometry filter KEPT candidate at 01:51:09.31 +64:52:47.1: ref_mag=13.54 +/- 0.04 new_mean_mag=10.6740 delta=2.87 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:50.53 +60:13:59.2: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:35.73 +57:57:38.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:50.53 +60:13:59.2: 13.61 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:35.73 +57:57:38.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.05
Forced photometry filter KEPT candidate at 02:02:50.53 +60:13:59.2: ref_mag=13.61 +/- 0.05 new_mean_mag=10.7524 delta=2.86 (need > 0.90)
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry filter KEPT candidate at 01:26:35.73 +57:57:38.8: ref_mag=13.34 +/- 0.03 new_mean_mag=10.7011 delta=2.64 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:48.49 +64:12:26.3: 11.87 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:40.21 +61:07:38.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:40.21 +61:07:38.8: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.06
Forced photometry filter KEPT candidate at 01:32:40.21 +61:07:38.8: ref_mag=13.74 +/- 0.06 new_mean_mag=10.7584 delta=2.99 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:48.49 +64:12:26.3: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.05
Forced photometry filter KEPT candidate at 01:18:48.49 +64:12:26.3: ref_mag=13.50 +/- 0.05 new_mean_mag=10.8421 delta=2.66 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:56.35 +58:41:02.1: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:56.35 +58:41:02.1: 13.87 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.07
Forced photometry filter KEPT candidate at 01:11:56.35 +58:41:02.1: ref_mag=13.87 +/- 0.07 new_mean_mag=10.8173 delta=3.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.79 +61:04:14.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:58.38 +60:30:24.8: 12.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.35 +59:18:56.6: 13.07 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:05.79 +61:04:14.5: 13.87 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:58.38 +60:30:24.8: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.06
Forced photometry filter KEPT candidate at 01:38:05.79 +61:04:14.5: ref_mag=13.87 +/- 0.06 new_mean_mag=10.9232 delta=2.95 (need > 0.90)
Forced photometry reference-image weighted average: 13.66 +/- 0.06
Forced photometry filter KEPT candidate at 01:14:58.38 +60:30:24.8: ref_mag=13.66 +/- 0.06 new_mean_mag=10.8097 delta=2.85 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.35 +59:18:56.6: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter KEPT candidate at 01:06:55.35 +59:18:56.6: ref_mag=13.82 +/- 0.05 new_mean_mag=10.8372 delta=2.99 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.42 +64:22:26.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.42 +64:22:26.5: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Forced photometry filter KEPT candidate at 01:31:48.42 +64:22:26.5: ref_mag=13.99 +/- 0.06 new_mean_mag=10.9564 delta=3.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:02.26 +60:36:56.0: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:02.26 +60:36:56.0: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter KEPT candidate at 02:16:02.26 +60:36:56.0: ref_mag=13.75 +/- 0.04 new_mean_mag=10.9431 delta=2.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:38.83 +58:10:50.9: 13.01 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:38.83 +58:10:50.9: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 01:13:38.83 +58:10:50.9: ref_mag=13.78 +/- 0.04 new_mean_mag=10.8503 delta=2.93 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:03.24 +58:57:14.1: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:03.24 +58:57:14.1: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 01:43:03.24 +58:57:14.1: ref_mag=13.71 +/- 0.04 new_mean_mag=10.9498 delta=2.76 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.40 +59:01:14.8: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.40 +59:01:14.8: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.06
Forced photometry filter KEPT candidate at 01:26:05.40 +59:01:14.8: ref_mag=13.95 +/- 0.06 new_mean_mag=11.0412 delta=2.91 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:17.42 +63:24:22.4: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:17.42 +63:24:22.4: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.06
Forced photometry filter KEPT candidate at 01:42:17.42 +63:24:22.4: ref_mag=14.02 +/- 0.06 new_mean_mag=11.1621 delta=2.86 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:30.39 +59:06:33.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:30.39 +59:06:33.9: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter KEPT candidate at 01:54:30.39 +59:06:33.9: ref_mag=13.69 +/- 0.04 new_mean_mag=11.0710 delta=2.62 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:35.05 +58:41:32.4: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:35.05 +58:41:32.4: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Forced photometry filter KEPT candidate at 01:48:35.05 +58:41:32.4: ref_mag=14.03 +/- 0.06 new_mean_mag=11.1055 delta=2.93 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:15.59 +61:53:38.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:15.59 +61:53:38.5: 14.03 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.16
Forced photometry filter KEPT candidate at 01:44:15.59 +61:53:38.5: ref_mag=14.03 +/- 0.16 new_mean_mag=11.1633 delta=2.87 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:28.43 +59:41:37.2: 12.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:28.43 +59:41:37.2: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.06
Forced photometry filter KEPT candidate at 01:26:28.43 +59:41:37.2: ref_mag=14.06 +/- 0.06 new_mean_mag=11.1768 delta=2.88 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:39.85 +60:37:33.1: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:39.85 +60:37:33.1: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.07
Forced photometry filter KEPT candidate at 01:37:39.85 +60:37:33.1: ref_mag=14.06 +/- 0.07 new_mean_mag=11.3836 delta=2.68 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:09.98 +60:03:40.1: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:09.98 +60:03:40.1: 14.37 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.08
Forced photometry filter KEPT candidate at 01:49:09.98 +60:03:40.1: ref_mag=14.37 +/- 0.08 new_mean_mag=11.3125 delta=3.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:18.46 +62:21:00.6: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:18.46 +62:21:00.6: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
Forced photometry filter KEPT candidate at 02:14:18.46 +62:21:00.6: ref_mag=14.09 +/- 0.06 new_mean_mag=11.5692 delta=2.52 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:22.35 +58:47:11.2: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:22.35 +58:47:11.2: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry filter KEPT candidate at 02:18:22.35 +58:47:11.2: ref_mag=13.34 +/- 0.03 new_mean_mag=9.4001 delta=3.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:44.34 +60:46:19.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.34 +60:46:19.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 01:33:44.34 +60:46:19.4: ref_mag=13.40 +/- 0.03 new_mean_mag=10.9389 delta=2.46 (need > 0.90)
Adding exclusion_list_local.txt__out125111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out273038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out273192.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 104s
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: 49s
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Considering the candidate 247636_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247636_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:09:23.41 +61:36:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247638_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247638_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247644_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247644_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247653_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247653_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247659_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247659_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247665_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247665_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:30:06.60 +61:51:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247668_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247668_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247670_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247670_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247673_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247673_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247679_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247679_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247680_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247680_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247682_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247682_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247684_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247684_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247688_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247688_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247690_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247690_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247694_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247694_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247695_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247695_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247696_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247696_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:33:35.22 +59:56:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247697_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247697_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247698_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247698_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247699_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247699_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247702_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247702_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247703_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247703_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247705_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247705_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247706_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247706_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247710_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247710_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:29:22.56 +63:18:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247711_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247711_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247716_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247716_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247718_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247718_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247719_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247719_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247720_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247720_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:39:24.03 +58:23:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247721_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247721_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247722_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247722_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 247729_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247729_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247730_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247730_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247731_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247731_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 247736_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247736_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:32:21.86 +60:27:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247738_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247738_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:09:47.57 +58:11:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247742_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247742_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:19:23.95 +58:26:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247743_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247743_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:01:30.76 +65:05:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247747_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247747_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247750_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247750_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:07:33.93 +60:52:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247752_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247752_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247753_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247753_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247756_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247756_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:10:37.34 +57:22:42.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247760_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247760_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:05:57.24 +63:03:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247763_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247763_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:14:45.25 +60:30:05.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247766_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247766_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:25:15.26 +64:40:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247768_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247768_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247769_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247769_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:43:51.70 +61:54:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247770_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247770_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:12:41.00 +61:20:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247772_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247772_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:07:07.99 +57:44:36.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247773_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247773_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247774_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247774_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:15:55.89 +58:23:29.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247776_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247776_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:55:14.48 +59:32:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247778_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247778_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247779_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247779_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247780_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247780_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247781_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247781_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:43:59.15 +61:55:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247784_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247784_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247787_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 247787_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:22:08.22 +60:22:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247788_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 247788_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248759_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 248759_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251857_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 251857_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:44:02.09 +61:53:56.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251924_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 251924_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:46:08.54 +61:12:16.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251956_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 251956_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252462_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 252462_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:38:00.42 +57:56:45.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252625_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 252625_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:19:11.02 +58:20:31.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253106_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 253106_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:17:59.10 +57:47:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254389_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 254389_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:26:46.64 +57:46:54.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255063_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 255063_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:25:42.68 +65:40:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255606_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 255606_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:28:15.31 +58:44:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255976_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 255976_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:58:16.21 +59:38:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256400_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 256400_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:05:03.52 +64:21:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256681_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 256681_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:26:40.95 +60:46:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256740_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 256740_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:18:14.13 +61:44:37.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257383_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 257383_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:44:17.64 +61:53:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257642_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 257642_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:46:33.57 +61:16:47.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257782_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 257782_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:19:12.43 +65:35:57.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257823_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 257823_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:20:10.91 +58:12:09.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258183_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 258183_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:43:53.06 +61:53:15.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259228_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 259228_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:16:08.52 +58:49:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259241_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 259241_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:33:59.29 +58:28:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259395_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 259395_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:43:03.20 +58:08:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259396_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 259396_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:02:54.78 +64:25:00.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259520_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 259520_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:11:22.94 +61:21:06.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259533_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 259533_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:15:58.88 +63:12:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259714_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 259714_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:44:32.32 +58:45:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259865_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 259865_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:00:51.76 +58:31:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260190_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 260190_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:19:22.18 +58:19:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260259_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 260259_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:15:11.57 +60:07:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260463_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 260463_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:00:36.73 +58:30:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260509_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 260509_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:07:40.76 +63:30:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260717_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 260717_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:42:33.06 +63:52:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260983_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 260983_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:44:27.92 +60:41:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261071_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261071_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:16:36.12 +64:57:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261122_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261122_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:13:35.91 +57:52:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261366_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261366_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:34:10.29 +62:09:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261462_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261462_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:46:03.27 +61:12:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261674_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261674_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:44:01.22 +61:52:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261764_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261764_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:35:50.48 +61:27:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261831_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261831_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:48:38.24 +61:49:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261882_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261882_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:42:28.26 +58:17:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261892_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261892_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:33:23.04 +57:44:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261896_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 261896_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:39:56.79 +60:52:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262077_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262077_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:11:50.14 +59:02:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262105_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262105_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:19:03.64 +63:57:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262160_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262160_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:35:54.17 +60:13:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262340_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262340_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:58:04.16 +57:58:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262395_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262395_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:16:05.03 +58:49:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262398_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 262398_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 262494_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262494_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:15:34.13 +59:17:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262741_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262741_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:04:26.62 +65:05:53.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262758_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262758_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:10:23.63 +60:01:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262780_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262780_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:39:24.52 +63:23:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262798_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 262798_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:58:39.90 +59:15:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263038_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263038_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:06:23.50 +62:44:03.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263065_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263065_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:54:18.69 +63:38:03.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 263167_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263167_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:38:11.87 +61:01:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263271_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263271_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:38:08.40 +61:03:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263439_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263439_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:06:45.23 +59:50:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263456_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263456_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:19:41.49 +62:51:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263475_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263475_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:37:13.81 +58:38:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263541_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 263541_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 263659_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263659_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:29:33.01 +63:19:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263704_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263704_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:47:18.61 +63:38:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263709_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263709_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:16:24.19 +58:04:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263793_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 263793_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:37:13.06 +58:38:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264085_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 264085_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 264266_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264266_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:49:34.17 +61:03:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264280_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264280_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:23:17.09 +58:25:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264324_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264324_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:14:00.66 +59:02:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264451_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264451_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:38:33.69 +60:47:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264567_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 264567_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 264587_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264587_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:01:38.74 +61:45:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264610_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 264610_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 264697_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264697_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:13:30.10 +58:34:25.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 264850_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 264850_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 264878_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 264878_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 264962_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264962_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:48:39.89 +59:09:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264968_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264968_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 264971_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264971_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:23:07.53 +61:11:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264999_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 264999_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:16:02.16 +58:49:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265012_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 265012_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:43:12.66 +64:00:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265020_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 265020_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:44:56.44 +59:46:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265047_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 265047_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:46:50.82 +60:39:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265199_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 265199_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:41:50.89 +61:02:08.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265323_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 265323_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:31:32.37 +61:02:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265495_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 265495_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:10:31.60 +59:59:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265550_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 265550_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:20:40.51 +60:23:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265960_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 265960_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:54:34.58 +59:52:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266053_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266053_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:42:26.61 +59:34:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266141_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266141_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:01:15.20 +59:23:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266145_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 266145_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
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Considering the candidate 266367_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266367_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:55:52.88 +64:15:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266444_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266444_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:38:06.32 +58:10:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266464_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266464_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:37:41.38 +58:37:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266513_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266513_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:59:05.88 +59:55:34.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266538_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266538_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:02:53.99 +60:15:41.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266679_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266679_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:35:01.14 +60:22:17.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266728_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266728_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:42:54.86 +64:01:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266939_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 266939_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:21:28.98 +63:55:32.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266988_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 266988_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267116_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 267116_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267229_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 267229_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267296_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 267296_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:14:00.27 +61:42:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267426_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 267426_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:18:04.16 +65:36:26.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267461_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 267461_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:46:18.34 +60:59:19.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267515_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 267515_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:27:56.31 +62:46:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267932_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 267932_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268075_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 268075_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268105_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 268105_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268608_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 268608_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268694_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 268694_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268732_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 268732_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:54:06.09 +61:05:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269295_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 269295_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:49:06.16 +65:23:44.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269321_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 269321_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269344_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 269344_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:14:21.72 +59:59:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269347_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 269347_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269698_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 269698_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:17:01.81 +63:21:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269997_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 269997_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270138_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 270138_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271155_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 271155_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:56:25.29 +62:05:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271205_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 271205_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:36:07.39 +59:27:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272351_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 272351_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272526_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 272526_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273038_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 273038_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273192_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 273192_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 70271_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:20:32.44 +62:32:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153703_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 153703_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125111_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
Preparing report for the candidate 125111_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 112593_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:21:55.12 +61:20:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 72532_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:45:35.63 +63:07:04.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 76113_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 02:02:02.11 +62:41:31.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107571_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 107571_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
Rejecting candidate due to large distance (37.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427
The candidate 39378_fd_Cas-03-Q2b1x1_2026-05-08_04-59-00_20.00sec_-4.90C_LIGHT_0427 did not pass the final checks
**** FOUND 01:47:55.55 +64:32:54.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 157s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:33:44.34 +60:46:19.4
02:18:22.35 +58:47:11.2
01:33:12.81 +61:16:55.5
01:20:42.13 +59:35:06.2
01:36:49.01 +62:46:51.7
01:47:51.35 +61:11:12.5
01:06:13.05 +59:33:45.7
01:33:19.85 +62:33:19.9
02:20:39.63 +62:47:12.4
01:11:18.15 +59:35:40.9
01:15:23.17 +61:11:41.3
01:08:39.06 +60:32:41.5
01:12:00.85 +64:42:19.1
01:33:01.63 +59:16:31.0
01:26:24.82 +58:10:11.4
01:47:54.48 +60:23:59.1
01:24:54.85 +59:41:47.6
01:07:39.23 +59:59:18.0
02:00:23.20 +64:54:52.3
01:29:02.66 +58:46:10.3
01:54:45.26 +57:45:51.6
02:07:25.22 +57:54:57.6
01:28:32.99 +61:12:18.8
01:43:26.09 +58:38:22.4
01:13:44.71 +57:24:50.8
01:09:22.07 +64:35:17.1
01:07:35.13 +57:33:10.4
01:32:05.66 +61:59:26.0
01:52:47.83 +58:10:25.5
01:37:09.79 +58:51:05.8
01:09:09.17 +61:37:28.2
01:17:15.30 +58:35:37.9
01:04:09.39 +63:14:43.6
01:31:22.94 +59:33:43.3
01:11:15.92 +61:08:30.7
01:25:26.50 +60:57:44.8
01:23:31.41 +58:41:47.7
01:20:24.26 +59:10:25.0
01:15:16.74 +57:28:04.8
01:52:08.93 +58:27:41.2
01:47:13.08 +57:44:19.0
01:35:37.81 +61:16:52.0
01:28:00.35 +61:19:59.2
01:46:38.35 +60:07:34.1
02:01:03.48 +64:43:34.6
01:51:09.31 +64:52:47.1
02:02:50.53 +60:13:59.2
01:26:35.73 +57:57:38.8
01:18:48.49 +64:12:26.3
01:32:40.21 +61:07:38.8
01:11:56.35 +58:41:02.1
01:38:05.79 +61:04:14.5
01:14:58.38 +60:30:24.8
01:06:55.35 +59:18:56.6
01:31:48.42 +64:22:26.5
02:16:02.26 +60:36:56.0
01:13:38.83 +58:10:50.9
01:43:03.24 +58:57:14.1
01:26:05.40 +59:01:14.8
01:42:17.42 +63:24:22.4
01:54:30.39 +59:06:33.9
01:48:35.05 +58:41:32.4
01:44:15.59 +61:53:38.5
01:26:28.43 +59:41:37.2
01:37:39.85 +60:37:33.1
01:49:09.98 +60:03:40.1
02:14:18.46 +62:21:00.6
########### Completed Cas-03-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 ####
01:33:12.81 +61:16:55.5
01:20:42.13 +59:35:06.2
01:36:49.01 +62:46:51.7
01:47:51.35 +61:11:12.5
01:06:13.05 +59:33:45.7
01:33:19.85 +62:33:19.9
02:20:39.63 +62:47:12.4
01:11:18.15 +59:35:40.9
01:15:23.17 +61:11:41.3
01:08:39.06 +60:32:41.5
01:12:00.85 +64:42:19.1
01:33:01.63 +59:16:31.0
01:26:24.82 +58:10:11.4
01:47:54.48 +60:23:59.1
01:24:54.85 +59:41:47.6
01:07:39.23 +59:59:18.0
02:00:23.20 +64:54:52.3
01:29:02.66 +58:46:10.3
01:54:45.26 +57:45:51.6
02:07:25.22 +57:54:57.6
01:28:32.99 +61:12:18.8
01:43:26.09 +58:38:22.4
01:13:44.71 +57:24:50.8
01:09:22.07 +64:35:17.1
01:07:35.13 +57:33:10.4
01:32:05.66 +61:59:26.0
01:52:47.83 +58:10:25.5
01:37:09.79 +58:51:05.8
01:09:09.17 +61:37:28.2
01:17:15.30 +58:35:37.9
01:04:09.39 +63:14:43.6
01:31:22.94 +59:33:43.3
01:11:15.92 +61:08:30.7
01:25:26.50 +60:57:44.8
01:23:31.41 +58:41:47.7
01:20:24.26 +59:10:25.0
01:15:16.74 +57:28:04.8
01:52:08.93 +58:27:41.2
01:47:13.08 +57:44:19.0
01:35:37.81 +61:16:52.0
01:28:00.35 +61:19:59.2
01:46:38.35 +60:07:34.1
02:01:03.48 +64:43:34.6
01:51:09.31 +64:52:47.1
02:02:50.53 +60:13:59.2
01:26:35.73 +57:57:38.8
01:18:48.49 +64:12:26.3
01:32:40.21 +61:07:38.8
01:11:56.35 +58:41:02.1
01:38:05.79 +61:04:14.5
01:14:58.38 +60:30:24.8
01:06:55.35 +59:18:56.6
01:31:48.42 +64:22:26.5
02:16:02.26 +60:36:56.0
01:13:38.83 +58:10:50.9
01:43:03.24 +58:57:14.1
01:26:05.40 +59:01:14.8
01:42:17.42 +63:24:22.4
01:54:30.39 +59:06:33.9
01:48:35.05 +58:41:32.4
01:44:15.59 +61:53:38.5
01:26:28.43 +59:41:37.2
01:37:39.85 +60:37:33.1
01:49:09.98 +60:03:40.1
02:14:18.46 +62:21:00.6
02:18:22.35 +58:47:11.2
01:33:44.34 +60:46:19.4
###################################################################################
01:33:12.81 +61:16:55.5 -- not an asteroid (will add it to exclusion list)
01:20:42.13 +59:35:06.2 -- not an asteroid (will add it to exclusion list)
01:36:49.01 +62:46:51.7 -- not an asteroid (will add it to exclusion list)
01:47:51.35 +61:11:12.5 -- not an asteroid (will add it to exclusion list)
01:06:13.05 +59:33:45.7 -- not an asteroid (will add it to exclusion list)
01:33:19.85 +62:33:19.9 -- not an asteroid (will add it to exclusion list)
02:20:39.63 +62:47:12.4 -- not an asteroid (will add it to exclusion list)
01:11:18.15 +59:35:40.9 -- not an asteroid (will add it to exclusion list)
01:15:23.17 +61:11:41.3 -- not an asteroid (will add it to exclusion list)
01:08:39.06 +60:32:41.5 -- not an asteroid (will add it to exclusion list)
01:12:00.85 +64:42:19.1 -- not an asteroid (will add it to exclusion list)
01:33:01.63 +59:16:31.0 -- not an asteroid (will add it to exclusion list)
01:26:24.82 +58:10:11.4 -- not an asteroid (will add it to exclusion list)
01:47:54.48 +60:23:59.1 -- not an asteroid (will add it to exclusion list)
01:24:54.85 +59:41:47.6 -- not an asteroid (will add it to exclusion list)
01:07:39.23 +59:59:18.0 -- not an asteroid (will add it to exclusion list)
02:00:23.20 +64:54:52.3 -- not an asteroid (will add it to exclusion list)
01:29:02.66 +58:46:10.3 -- not an asteroid (will add it to exclusion list)
01:54:45.26 +57:45:51.6 -- not an asteroid (will add it to exclusion list)
02:07:25.22 +57:54:57.6 -- not an asteroid (will add it to exclusion list)
01:28:32.99 +61:12:18.8 -- not an asteroid (will add it to exclusion list)
01:43:26.09 +58:38:22.4 -- not an asteroid (will add it to exclusion list)
01:13:44.71 +57:24:50.8 -- not an asteroid (will add it to exclusion list)
01:09:22.07 +64:35:17.1 -- not an asteroid (will add it to exclusion list)
01:07:35.13 +57:33:10.4 -- not an asteroid (will add it to exclusion list)
01:32:05.66 +61:59:26.0 -- not an asteroid (will add it to exclusion list)
01:52:47.83 +58:10:25.5 -- not an asteroid (will add it to exclusion list)
01:37:09.79 +58:51:05.8 -- not an asteroid (will add it to exclusion list)
01:09:09.17 +61:37:28.2 -- not an asteroid (will add it to exclusion list)
01:17:15.30 +58:35:37.9 -- not an asteroid (will add it to exclusion list)
01:04:09.39 +63:14:43.6 -- not an asteroid (will add it to exclusion list)
01:31:22.94 +59:33:43.3 -- not an asteroid (will add it to exclusion list)
01:11:15.92 +61:08:30.7 -- not an asteroid (will add it to exclusion list)
01:25:26.50 +60:57:44.8 -- not an asteroid (will add it to exclusion list)
01:23:31.41 +58:41:47.7 -- not an asteroid (will add it to exclusion list)
01:20:24.26 +59:10:25.0 -- not an asteroid (will add it to exclusion list)
01:15:16.74 +57:28:04.8 -- not an asteroid (will add it to exclusion list)
01:52:08.93 +58:27:41.2 -- not an asteroid (will add it to exclusion list)
01:47:13.08 +57:44:19.0 -- not an asteroid (will add it to exclusion list)
01:35:37.81 +61:16:52.0 -- not an asteroid (will add it to exclusion list)
01:28:00.35 +61:19:59.2 -- not an asteroid (will add it to exclusion list)
01:46:38.35 +60:07:34.1 -- not an asteroid (will add it to exclusion list)
02:01:03.48 +64:43:34.6 -- not an asteroid (will add it to exclusion list)
01:51:09.31 +64:52:47.1 -- not an asteroid (will add it to exclusion list)
02:02:50.53 +60:13:59.2 -- not an asteroid (will add it to exclusion list)
01:26:35.73 +57:57:38.8 -- not an asteroid (will add it to exclusion list)
01:18:48.49 +64:12:26.3 -- not an asteroid (will add it to exclusion list)
01:32:40.21 +61:07:38.8 -- not an asteroid (will add it to exclusion list)
01:11:56.35 +58:41:02.1 -- not an asteroid (will add it to exclusion list)
01:38:05.79 +61:04:14.5 -- not an asteroid (will add it to exclusion list)
01:14:58.38 +60:30:24.8 -- not an asteroid (will add it to exclusion list)
01:06:55.35 +59:18:56.6 -- not an asteroid (will add it to exclusion list)
01:31:48.42 +64:22:26.5 -- not an asteroid (will add it to exclusion list)
02:16:02.26 +60:36:56.0 -- not an asteroid (will add it to exclusion list)
01:13:38.83 +58:10:50.9 -- not an asteroid (will add it to exclusion list)
01:43:03.24 +58:57:14.1 -- not an asteroid (will add it to exclusion list)
01:26:05.40 +59:01:14.8 -- not an asteroid (will add it to exclusion list)
01:42:17.42 +63:24:22.4 -- not an asteroid (will add it to exclusion list)
01:54:30.39 +59:06:33.9 -- not an asteroid (will add it to exclusion list)
01:48:35.05 +58:41:32.4 -- not an asteroid (will add it to exclusion list)
01:44:15.59 +61:53:38.5 -- not an asteroid (will add it to exclusion list)
01:26:28.43 +59:41:37.2 -- not an asteroid (will add it to exclusion list)
01:37:39.85 +60:37:33.1 -- not an asteroid (will add it to exclusion list)
01:49:09.98 +60:03:40.1 -- not an asteroid (will add it to exclusion list)
02:14:18.46 +62:21:00.6 -- not an asteroid (will add it to exclusion list)
02:18:22.35 +58:47:11.2 -- not an asteroid (will add it to exclusion list)
01:33:44.34 +60:46:19.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:04:09.39 +63:14:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:13.05 +59:33:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.35 +59:18:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:35.13 +57:33:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.23 +59:59:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:39.06 +60:32:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:09.17 +61:37:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.07 +64:35:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:15.92 +61:08:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:18.15 +59:35:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:56.35 +58:41:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:00.85 +64:42:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:38.83 +58:10:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:44.71 +57:24:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:58.38 +60:30:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:16.74 +57:28:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:23.17 +61:11:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:15.30 +58:35:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:48.49 +64:12:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:24.26 +59:10:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:42.13 +59:35:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:31.41 +58:41:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:54.85 +59:41:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:26.50 +60:57:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.40 +59:01:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:24.82 +58:10:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:28.43 +59:41:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:35.73 +57:57:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:00.35 +61:19:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:32.99 +61:12:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:02.66 +58:46:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:22.94 +59:33:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.42 +64:22:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:05.66 +61:59:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:40.21 +61:07:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:01.63 +59:16:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:12.81 +61:16:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:19.85 +62:33:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:44.34 +60:46:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:37.81 +61:16:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:49.01 +62:46:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:09.79 +58:51:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:39.85 +60:37:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:05.79 +61:04:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:17.42 +63:24:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:03.24 +58:57:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:26.09 +58:38:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:15.59 +61:53:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.35 +60:07:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:13.08 +57:44:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:51.35 +61:11:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:54.48 +60:23:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:35.05 +58:41:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:09.98 +60:03:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:09.31 +64:52:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:08.93 +58:27:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:47.83 +58:10:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:30.39 +59:06:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:45.26 +57:45:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:23.20 +64:54:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:03.48 +64:43:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:50.53 +60:13:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:25.22 +57:54:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:18.46 +62:21:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:02.26 +60:36:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:22.35 +58:47:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:39.63 +62:47:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:04:09.39 +63:14:43.6 -- not a known variable star
01:06:13.05 +59:33:45.7 -- not a known variable star
01:06:55.35 +59:18:56.6 -- not a known variable star
01:07:35.13 +57:33:10.4 -- not a known variable star
01:07:39.23 +59:59:18.0 -- not a known variable star
01:08:39.06 +60:32:41.5 -- not a known variable star
01:09:09.17 +61:37:28.2 -- a known variable star
01:09:22.07 +64:35:17.1 -- not a known variable star
01:11:15.92 +61:08:30.7 -- a known variable star
01:11:18.15 +59:35:40.9 -- not a known variable star
01:11:56.35 +58:41:02.1 -- not a known variable star
01:12:00.85 +64:42:19.1 -- a known variable star
01:13:38.83 +58:10:50.9 -- not a known variable star
01:13:44.71 +57:24:50.8 -- not a known variable star
01:14:58.38 +60:30:24.8 -- a known variable star
01:15:16.74 +57:28:04.8 -- not a known variable star
01:15:23.17 +61:11:41.3 -- not a known variable star
01:17:15.30 +58:35:37.9 -- not a known variable star
01:18:48.49 +64:12:26.3 -- not a known variable star
01:20:24.26 +59:10:25.0 -- not a known variable star
01:20:42.13 +59:35:06.2 -- not a known variable star
01:23:31.41 +58:41:47.7 -- a known variable star
01:24:54.85 +59:41:47.6 -- not a known variable star
01:25:26.50 +60:57:44.8 -- not a known variable star
01:26:05.40 +59:01:14.8 -- not a known variable star
01:26:24.82 +58:10:11.4 -- a known variable star
01:26:28.43 +59:41:37.2 -- not a known variable star
01:26:35.73 +57:57:38.8 -- not a known variable star
01:28:00.35 +61:19:59.2 -- not a known variable star
01:28:32.99 +61:12:18.8 -- not a known variable star
01:29:02.66 +58:46:10.3 -- not a known variable star
01:31:22.94 +59:33:43.3 -- not a known variable star
01:31:48.42 +64:22:26.5 -- not a known variable star
01:32:05.66 +61:59:26.0 -- not a known variable star
01:32:40.21 +61:07:38.8 -- not a known variable star
01:33:01.63 +59:16:31.0 -- not a known variable star
01:33:12.81 +61:16:55.5 -- not a known variable star
01:33:19.85 +62:33:19.9 -- not a known variable star
01:33:44.34 +60:46:19.4 -- not a known variable star
01:35:37.81 +61:16:52.0 -- a known variable star
01:36:49.01 +62:46:51.7 -- a known variable star
01:37:09.79 +58:51:05.8 -- a known variable star
01:37:39.85 +60:37:33.1 -- not a known variable star
01:38:05.79 +61:04:14.5 -- not a known variable star
01:42:17.42 +63:24:22.4 -- not a known variable star
01:43:03.24 +58:57:14.1 -- not a known variable star
01:43:26.09 +58:38:22.4 -- a known variable star
01:44:15.59 +61:53:38.5 -- not a known variable star
01:46:38.35 +60:07:34.1 -- not a known variable star
01:47:13.08 +57:44:19.0 -- a known variable star
01:47:51.35 +61:11:12.5 -- not a known variable star
01:47:54.48 +60:23:59.1 -- a known variable star
01:48:35.05 +58:41:32.4 -- not a known variable star
01:49:09.98 +60:03:40.1 -- not a known variable star
01:51:09.31 +64:52:47.1 -- a known variable star
01:52:08.93 +58:27:41.2 -- not a known variable star
01:52:47.83 +58:10:25.5 -- not a known variable star
01:54:30.39 +59:06:33.9 -- not a known variable star
01:54:45.26 +57:45:51.6 -- a known variable star
02:00:23.20 +64:54:52.3 -- not a known variable star
02:01:03.48 +64:43:34.6 -- not a known variable star
02:02:50.53 +60:13:59.2 -- a known variable star
02:07:25.22 +57:54:57.6 -- not a known variable star
02:14:18.46 +62:21:00.6 -- not a known variable star
02:16:02.26 +60:36:56.0 -- not a known variable star
02:18:22.35 +58:47:11.2 -- a known variable star
02:20:39.63 +62:47:12.4 -- not a known variable star
Found 51 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
67 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 67 (excluding asteroids and hot pixels, 51 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)2461168.91551087 -observatory V36
02:32:26.67 +14:01:11.4 Mercury (-1.5mag)
05:02:26.43 +23:59:33.7 Venus (-3.9mag)
01:21:22.02 +07:40:14.7 Mars (1.2mag)
07:25:13.53 +22:23:26.5 Jupiter (-2.0mag)
00:38:42.31 +01:47:13.0 Saturn (0.9mag)
03:52:46.17 +20:03:22.0 Uranus (5.8mag)
00:13:32.25 +00:01:23.5 Neptune (7.8mag)
20:34:14.57 -22:55:26.3 Pluto (14.5mag)
20:16:58.95 -23:28:01.3 Moon (-10.8mag)
-rw-r--r-- 1 apache apache 363 May 8 05:03 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461168.91551087:
07:25:09.23 +22:23:35.2 Io (5.9mag)
07:25:24.19 +22:22:59.3 Europa (6.0mag)
07:25:20.18 +22:23:04.6 Ganymede (5.5mag)
07:24:59.65 +22:23:51.8 Callisto (6.7mag)
07:27:23.17 +22:02:49.1 Himalia (15.5mag)
07:25:11.49 +22:23:31.0 Thebe (16.4mag)
07:27:51.40 +22:30:35.3 Elara (17.4mag)
07:25:35.99 +22:51:40.9 Pasiphae (17.6mag)
07:32:57.55 +22:23:11.5 Carme (18.7mag)
00:38:37.25 +01:47:06.6 Titan (8.7mag)
00:38:39.18 +01:47:18.6 Rhea (10.0mag)
00:38:24.25 +01:45:08.5 Iapetus (11.4mag)
00:38:46.98 +01:47:39.1 Hyperion (14.7mag)
00:39:58.99 +01:53:22.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 8 05:03 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461168.91551087:
16:51:02.11 -28:11:20.1 JWST
17:37:29.44 +38:31:28.8 Chandra
09:15:57.17 -52:54:32.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 8 05:03 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461168.91551087 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
07:20:14.15 +27:18:54.9 17.7mag P/2009 WX51 (Catalina)
18:55:48.17 -30:16:45.0 13.7mag P/2010 H2 (Vales)
05:24:40.58 -68:45:03.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:38:25.93 +31:37:15.4 17.4mag C/2017 K2 (PANSTARRS)
17:25:55.66 +13:00:41.4 17.7mag C/2021 G2 (ATLAS)
23:14:20.47 +30:13:12.4 17.1mag C/2022 E2 (ATLAS)
04:56:07.17 +26:34:18.1 16.2mag C/2022 N2 (PANSTARRS)
09:11:11.74 +31:53:19.7 16.4mag C/2022 QE78 (ATLAS)
08:36:46.14 +01:56:50.8 17.5mag C/2022 R6 (PANSTARRS)
18:45:48.53 +20:14:18.9 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:32:02.12 -11:12:18.1 17.5mag P/2023 B1 (PANSTARRS)
09:00:48.73 -08:39:52.6 17.9mag C/2023 F3 (ATLAS)
22:11:11.97 +64:23:10.9 17.6mag C/2023 H5 (Lemmon)
18:51:27.19 -04:25:09.2 13.9mag C/2023 R1 (PANSTARRS)
17:18:14.83 +88:18:31.0 17.9mag C/2023 X2 (Lemmon)
06:34:06.29 +63:35:55.1 17.4mag C/2024 A1 (ATLAS)
05:56:46.69 +23:50:53.5 12.3mag C/2024 E1 (Wierzchos)
16:02:40.80 +09:53:32.6 17.3mag C/2024 G6 (ATLAS)
20:23:32.69 +21:43:41.8 14.3mag C/2024 J3 (ATLAS)
03:47:25.61 -19:15:35.1 16.2mag C/2024 T5 (ATLAS)
05:36:53.44 +40:15:15.7 17.8mag C/2025 J1 (Borisov)
12:19:24.05 +52:53:07.5 16.2mag C/2025 L1 (ATLAS)
04:04:18.23 -30:12:26.1 18.0mag C/2025 Q3 (ATLAS)
05:16:40.19 -06:27:31.8 9.8mag C/2025 R3 (PANSTARRS)
12:45:23.02 +04:08:31.4 17.3mag C/2025 Y1 (ATLAS)
05:17:31.69 +01:28:20.1 17.4mag C/2026 A1 (MAPS)
00:57:38.40 +40:33:15.2 15.3mag C/2026 B2 (Sun-Gao)
19:26:09.42 -08:32:59.4 10.5mag 10P/Tempel
14:31:58.49 +00:15:21.3 16.0mag 24P/Schaumasse
10:59:09.78 -00:59:10.5 15.8mag 29P/Schwassmann-Wachmann
10:41:47.74 -02:49:58.5 17.4mag 43P/Wolf-Harrington
02:23:37.60 +21:09:36.2 17.4mag 47P/Ashbrook-Jackson
07:54:56.95 +31:53:54.0 16.9mag 63P/Wild
23:56:02.51 -08:57:26.9 15.7mag 65P/Gunn
05:06:48.95 +27:57:17.2 16.1mag 76P/West-Kohoutek-Ikemura
01:56:16.91 +12:26:50.0 14.1mag 78P/Gehrels
00:06:31.49 -02:52:38.4 14.9mag 88P/Howell
03:16:49.10 +25:56:53.4 15.1mag 93P/Lovas
05:40:16.84 +33:10:34.0 15.9mag 123P/West-Hartley
08:59:21.01 +28:08:29.7 16.3mag 124P/Mrkos
03:08:40.22 +16:42:40.8 16.4mag 128P/Shoemaker-Holt
03:31:59.54 +16:55:02.3 17.6mag 131P/Mueller
03:27:11.19 +18:46:00.4 11.1mag 141P/Machholz
03:32:00.03 +12:30:46.8 11.1mag 141P-A/Machholz
02:12:00.82 +08:32:38.1 10.7mag 141P-D/Machholz
02:34:43.59 -29:47:29.8 17.9mag 161P/Hartley-IRAS
02:06:15.91 +09:45:30.3 14.9mag 162P/SidingSpring
17:13:44.68 -11:11:50.4 16.1mag 235P/LINEAR
06:24:25.50 +35:47:56.0 17.1mag 240P/NEAT
07:52:13.03 -03:07:17.0 17.9mag 242P/Spahr
23:13:14.52 -14:13:22.6 17.2mag 260P/McNaught
02:46:53.37 +25:56:39.7 17.8mag 295P/LINEAR
15:31:40.45 +08:07:16.2 17.4mag 391P/Kowalski
07:45:23.14 +21:17:30.3 17.8mag 450P/LONEOS
06:10:10.52 +43:42:33.6 17.7mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K May 8 05:03 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
21:35:33.81 -14:05:16.30 2026-05-6.29 14.51
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:35:33.81 -14:05:16.30 2026-05-6.29 14.51
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
-rw-r--r-- 1 apache apache 188K May 8 05:03 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:21:22.210 -00:16:07.65 AT 2026kxu 2026-02-21.91 23.04
11:10:04.960 +03:00:11.06 AT 2026kxt 2026-02-21.77 22.61
13:22:39.150 +02:20:19.00 AT 2026kxs 2026-02-18.94 22.95
14:24:07.420 -01:46:56.77 AT 2026kxr 2026-02-12.87 22.64
10:25:02.950 +00:46:15.40 AT 2026kxq 2026-02-12.75 22.4
11:30:30.430 -01:03:47.47 AT 2026kxp 2026-02-10.85 22.79
10:35:18.870 +03:52:47.32 AT 2026kxo 2026-02-09.80 22.21
11:19:29.420 +02:06:33.76 AT 2026kxn 2026-02-06.89 21.88
10:54:26.610 +04:03:05.24 AT 2026kxm 2026-01-29.84 21.96
10:56:41.020 +03:32:12.55 AT 2026kxl 2026-01-26.81 22.56
13:15:43.480 +00:54:01.42 AT 2026kxk 2026-01-21.96 22.29
10:51:56.160 +02:19:18.12 AT 2026kxj 2026-01-20.86 22.35
14:26:48.440 +02:30:09.54 AT 2026kxi 2026-01-14.95 22.23
10:43:57.670 +01:30:50.24 AT 2026kxh 2026-01-14.79 22.42
13:23:50.230 -01:41:58.87 AT 2026kxg 2026-01-11.96 22.13
13:35:32.150 +04:23:37.08 AT 2026kxf 2026-01-10.97 21.84
13:21:21.710 +02:11:06.23 AT 2026kxe 2026-02-18.83 21.99
13:35:40.300 +02:19:57.82 AT 2026kxd 2026-02-11.88 22.78
20:34:18.052 -34:09:25.84 AT 2026kxc 2026-04-15.79 20.17
22:37:20.204 -11:55:44.02 AT 2026kxb 2026-04-25.79 18.91
-rw-r--r-- 1 apache apache 30K May 8 05:03 tns_transients_list.txt
