This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 11.21 00:21:39.71 +55:23:07.1
118.67739 -7.24028 galactic Cas Second-epoch detections are separated by 1.1" and 7.7 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 J005.3970+55.3821 | 00:21:39.71 +55:23:07.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.359+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:21:39.71 +55:23:07.1: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:21:39.71 +55:23:07.1: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 21 39.71 +55 23 07.1 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 J005.3970+55.3821,2461232.6967,11.21,0.05,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 J005.3970+55.3821 20260711.1967 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 11.20 00:27:38.39 +57:26:54.4
119.72121 -5.27487 galactic Cas Second-epoch detections are separated by 1.0" and 7.9 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 421876190610188032 | 00:27:37.13 +57:27:09.7 (Gaia DR3) | E (local) | 0.413236000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.381+/-0.027 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:38.39 +57:26:54.4: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:38.39 +57:26:54.4: 13.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 27 38.39 +57 26 54.4 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 421876190610188032,2461232.6967,11.20,0.05,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 421876190610188032 20260711.1967 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 11.02 00:30:23.31 +55:49:11.2
119.95663 -6.93032 galactic Cas Second-epoch detections are separated by 2.8" and 7.9 pix
The object was found in VSX13" Gaia DR3 421273280280788608
Type: ROT
# Max. Min./Amp. JD0 Period
15.310 G 15.340 G G
ATTENTION: measured mag 11.02 is 4.3 mag brighter than the VSX record maximum brightness 15.31 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:23.31 +55:49:11.2: 13.58 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:23.31 +55:49:11.2: 13.45 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.58 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 30 23.31 +55 49 11.2 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 421273280280788608,2461232.6967,11.02,0.05,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 421273280280788608 20260711.1967 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.96 00:17:42.12 +53:02:30.1
117.80241 -9.49373 galactic Cas Second-epoch detections are separated by 0.9" and 7.9 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 419225061920381568 | 00:17:40.63 +53:02:20.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.357+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:42.12 +53:02:30.1: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:42.12 +53:02:30.1: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 17 42.12 +53 02 30.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419225061920381568,2461232.6967,10.96,0.05,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
Gaia DR3 419225061920381568 20260711.1967 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 11.15 00:22:45.25 +50:48:14.6
118.30912 -11.81005 galactic Cas Second-epoch detections are separated by 2.5" and 8.2 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 394741102624962560 | 00:22:44.05 +50:47:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:22:45.25 +50:48:14.6: 13.65 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:22:45.25 +50:48:14.6: 13.42 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 22 45.25 +50 48 14.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394741102624962560,2461232.6967,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 394741102624962560 20260711.1967 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 11.09 23:58:11.83 +50:30:00.5
114.33806 -11.48110 galactic Cas Second-epoch detections are separated by 1.7" and 8.2 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 1940966472068395008 | 23:58:14.42 +50:29:39.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:11.83 +50:30:00.5: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:11.83 +50:30:00.5: 13.34 +/- 0.35 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 23 58 11.83 +50 30 00.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940966472068395008,2461232.6967,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940966472068395008 20260711.1967 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 11.09 00:26:10.87 +57:09:01.8
119.49564 -5.55264 galactic Cas Second-epoch detections are separated by 4.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421783762906643968 | 00:26:13.28 +57:09:11.4 (Gaia DR3) | E (local) | 5.808100000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:26:10.87 +57:09:01.8: 12.95 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:10.87 +57:09:01.8: 13.29 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 26 10.87 +57 09 01.8 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 421783762906643968,2461232.6967,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421783762906643968 20260711.1967 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.93 23:55:25.78 +50:00:50.5
113.79040 -11.86098 galactic Cas Second-epoch detections are separated by 2.1" and 8.0 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 | Large-amplitude variable Gaia DR2 1940921151571286272 | 23:55:27.71 +50:00:49.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: M0 (LAMOST DR5) J-Ks=0.387+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:55:25.78 +50:00:50.5: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:55:25.78 +50:00:50.5: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 23 55 25.78 +50 00 50.5 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
Large-amplitude variable Gaia DR2 1940921151571286272,2461232.6967,10.93,0.05,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
Large-amplitude variable Gaia DR2 1940921151571286272 20260711.1967 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 07 11.1967 2461232.6967 10.46 23:40:53.01 +58:05:25.0
113.69785 -3.51093 galactic Cas Second-epoch detections are separated by 0.4" and 7.2 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 J355.2216+58.0897 | 23:40:53.20 +58:05:23.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.345+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:40:53.01 +58:05:25.0: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:40:53.01 +58:05:25.0: 13.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 23 40 53.01 +58 05 25.0 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.2216+58.0897,2461232.6967,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.2216+58.0897 20260711.1967 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.66 00:28:47.70 +56:39:17.8
119.80627 -6.07932 galactic Cas Second-epoch detections are separated by 0.4" and 7.8 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 J007.1958+56.6564 | 00:28:47.70 +56:39:17.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.208+/-0.031 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:47.70 +56:39:17.8: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:47.70 +56:39:17.8: 13.33 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 28 47.70 +56 39 17.8 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 J007.1958+56.6564,2461232.6967,10.66,0.05,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
ATO J007.1958+56.6564 20260711.1967 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.73 00:02:42.03 +50:03:44.0
114.96827 -12.05441 galactic Cas Second-epoch detections are separated by 1.7" and 8.1 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 393899735717641344 | 00:02:44.33 +50:03:55.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:02:42.03 +50:03:44.0: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:02:42.03 +50:03:44.0: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 02 42.03 +50 03 44.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393899735717641344,2461232.6967,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 393899735717641344 20260711.1967 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.41 23:54:48.95 +50:53:17.5
113.89016 -10.98682 galactic Cas Second-epoch detections are separated by 2.6" and 7.7 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 1944027512436950528 | 23:54:50.28 +50:53:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.312+/-0.031 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:48.95 +50:53:17.5: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:54:48.95 +50:53:17.5: 13.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 23 54 48.95 +50 53 17.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944027512436950528,2461232.6967,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944027512436950528 20260711.1967 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.47 00:07:23.03 +50:57:10.1
115.88203 -11.31492 galactic Cas Second-epoch detections are separated by 1.8" and 7.9 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 395321060653737344 | 00:07:26.38 +50:56:48.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=-0.038+/-0.030 (B)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:23.03 +50:57:10.1: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:23.03 +50:57:10.1: 13.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 07 23.03 +50 57 10.1 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395321060653737344,2461232.6967,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 395321060653737344 20260711.1967 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.40 00:19:52.71 +51:31:14.3
117.93942 -11.04492 galactic Cas Second-epoch detections are separated by 1.7" and 8.0 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 395057384021349504 | 00:19:54.20 +51:31:31.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.134+/-0.028 (A)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:52.71 +51:31:14.3: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:52.71 +51:31:14.3: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 19 52.71 +51 31 14.3 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395057384021349504,2461232.6967,10.40,0.05,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
Gaia DR3 395057384021349504 20260711.1967 10.40CV 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 07 11.1967 2461232.6967 10.32 23:57:09.55 +50:24:08.7
114.15219 -11.54174 galactic Cas Second-epoch detections are separated by 1.4" and 7.8 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 1940965132036769408 | 23:57:07.17 +50:23:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.815+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:09.55 +50:24:08.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:09.55 +50:24:08.7: 13.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 23 57 09.55 +50 24 08.7 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940965132036769408,2461232.6967,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1940965132036769408 20260711.1967 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.12 00:24:30.34 +52:14:19.4
118.74563 -10.41398 galactic Cas Second-epoch detections are separated by 0.3" and 7.9 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 418943479557768960 | 00:24:30.45 +52:14:33.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.027 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:24:30.34 +52:14:19.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:24:30.34 +52:14:19.4: 13.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 24 30.34 +52 14 19.4 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 418943479557768960,2461232.6967,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 418943479557768960 20260711.1967 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 9.97 00:28:10.81 +56:29:42.5
119.70707 -6.23091 galactic Cas Second-epoch detections are separated by 0.9" and 7.7 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 421682195525573504 | 00:28:13.11 +56:30:07.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:10.81 +56:29:42.5: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:10.81 +56:29:42.5: 13.41 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 28 10.81 +56 29 42.5 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421682195525573504,2461232.6967,9.97,0.05,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
Gaia DR3 421682195525573504 20260711.1967 9.97CV 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 07 11.1967 2461232.6967 9.40 00:19:34.61 +50:02:30.0
117.70165 -12.50624 galactic Cas Second-epoch detections are separated by 0.7" and 8.0 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 394497835678366592 | 00:19:36.25 +50:02:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1958PMcCO..13b....V AG+49 48 J-Ks=0.252+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:34.61 +50:02:30.0: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:34.61 +50:02:30.0: 13.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 19 34.61 +50 02 30.0 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 394497835678366592,2461232.6967,9.40,0.05,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
Gaia DR3 394497835678366592 20260711.1967 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 07 11.1967 2461232.6967 9.99 00:14:07.25 +51:33:29.2
117.04112 -10.88631 galactic Cas Second-epoch detections are separated by 0.7" and 8.0 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 J001410.11+513334.1 | 00:14:10.11 +51:33:34.1 (Gaia DR3) | SR (local) | 144.000000000000 (local) | Gaia3var=VARIABLE SpType: MS 1984PW&SO...3....1S CSS 5 J-Ks=0.345+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:14:07.25 +51:33:29.2: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:14:07.25 +51:33:29.2: 13.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 14 07.25 +51 33 29.2 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J001410.11+513334.1,2461232.6967,9.99,0.05,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
ASASSN-V J001410.11+513334.1 20260711.1967 9.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.15 00:28:41.93 +57:00:51.0
119.82504 -5.72035 galactic Cas Second-epoch detections are separated by 0.5" and 7.8 pix
The object was found in VSX24" Gaia DR3 421813484080843904
Type: E
# Max. Min./Amp. JD0 Period
10.900 G 10.960 G 3.371510000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:41.93 +57:00:51.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:41.93 +57:00:51.0: 13.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 28 41.93 +57 00 51.0 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421813484080843904,2461232.6967,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421813484080843904 20260711.1967 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.54 00:25:23.70 +55:26:50.8
119.21503 -7.23624 galactic Cas Second-epoch detections are separated by 0.9" and 7.6 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 421200575075768832 | 00:25:26.59 +55:26:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.645+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:23.70 +55:26:50.8: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:23.70 +55:26:50.8: 13.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 25 23.70 +55 26 50.8 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421200575075768832,2461232.6967,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421200575075768832 20260711.1967 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.76 00:13:17.61 +50:25:36.1
116.73798 -11.98575 galactic Cas Second-epoch detections are separated by 1.6" and 8.0 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 395237360330004736 | 00:13:20.94 +50:25:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.381+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:13:17.61 +50:25:36.1: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:13:17.61 +50:25:36.1: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 13 17.61 +50 25 36.1 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
Gaia DR3 395237360330004736,2461232.6967,10.76,0.05,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 395237360330004736 20260711.1967 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 10.98 00:12:08.66 +50:38:18.9
116.58668 -11.74843 galactic Cas Second-epoch detections are separated by 0.9" and 7.9 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 395243338924336128 | 00:12:12.52 +50:37:59.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.270+/-0.031 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:12:08.66 +50:38:18.9: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:12:08.66 +50:38:18.9: 13.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 12 08.66 +50 38 18.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395243338924336128,2461232.6967,10.98,0.05,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
Gaia DR3 395243338924336128 20260711.1967 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
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 11.08 00:11:16.72 +50:50:57.7
116.48232 -11.51879 galactic Cas Second-epoch detections are separated by 1.2" and 7.9 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 | 00:11:16.72 +50:50:57.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:11:16.72 +50:50:57.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:11:16.72 +50:50:57.7: 13.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 11 16.72 +50 50 57.7 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,2461232.6967,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260711.1967 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 11.01 00:06:29.52 +50:07:47.8
115.59219 -12.10018 galactic Cas Second-epoch detections are separated by 0.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.6233+50.1303 | 00:06:26.54 +50:07:38.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.156+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:06:29.52 +50:07:47.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:06:29.52 +50:07:47.8: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 06 29.52 +50 07 47.8 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 J001.6233+50.1303,2461232.6967,11.01,0.05,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
ATO J001.6233+50.1303 20260711.1967 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 07 11.1967 2461232.6967 11.11 00:04:13.36 +51:32:55.3
115.49517 -10.64000 galactic Cas Second-epoch detections are separated by 0.5" and 7.9 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 395541237856954880 | 00:04:16.83 +51:32:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.757+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:04:13.36 +51:32:55.3: 13.11 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:04:13.36 +51:32:55.3: 13.08 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 04 13.36 +51 32 55.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395541237856954880,2461232.6967,11.11,0.05,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
Gaia DR3 395541237856954880 20260711.1967 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 11.1967 2461232.6967 11.03 00:19:32.89 +57:40:49.0
118.66354 -4.92694 galactic Cas Second-epoch detections are separated by 1.4" and 7.8 pix
The object was found in VSX25" Gaia DR3 422043827475326208
Type: S
# Max. Min./Amp. JD0 Period
16.100 G 16.930 G F
ATTENTION: measured mag 11.03 is 5.1 mag brighter than the VSX record maximum brightness 16.10 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:32.89 +57:40:49.0: 13.31 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:32.89 +57:40:49.0: 13.31 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.31 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 11.1967* 00 19 32.89 +57 40 49.0 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
Gaia DR3 422043827475326208,2461232.6967,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 422043827475326208 20260711.1967 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
First image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461232.69704418 11.07.2026 04:43:34.617 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.79
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: 8 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): 17073
Objects passed selection criteria: 16986
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 10646.8
Average stars matched: 10324.5 (96.9733 %)
Memory usage VmPeak: 123496 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 10 19:09:57 CDT 2026
VaST build number 1.0rc89-143-g13f85f26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 11 00:53:41 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
First image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461232.69704418 11.07.2026 04:43:34.617 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 47 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): 132073
Objects passed selection criteria: 131654
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 88940.5
Average stars matched: 85647 (96.297 %)
Memory usage VmPeak: 1967860 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 10 19:09:57 CDT 2026
VaST build number 1.0rc89-143-g13f85f26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 11 00:59:12 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-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461232.69634522
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Image size: 927.0'x616.4' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:01.466 +54:00:23.28 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
Image size: 939.0'x624.3' 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: 23:59:25.538 +54:00:50.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 23:59:25.538 +54:00:50.88
Angular distance between the image centers 0.0883 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Image size: 939.0'x624.3' 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: 23:59:29.589 +54:01:19.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 23:59:29.589 +54:01:19.49
Angular distance between the image centers 0.0796 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:25.538 +54:00:50.88
Second-epoch second image center 23:59:29.589 +54:01:19.49
Angular distance between the image centers 0.01271 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits &> /tmp/tmp.DIIhyVtZ1r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits &> /tmp/tmp.i7zfPQ5I5d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits &> /tmp/tmp.1CkBazGYVX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits &> /tmp/tmp.aEdD8Wj29y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 23386 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0031 to 359.9999 deg, Dec +48.2162 to +59.2586 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0031 to 359.9999 deg, Dec 48.2162 to 59.2586 deg
Loaded 153985 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 53 out of 58 total matches.
Matched with Tycho-2 58 out of 23386 detected stars.
ERROR: only 53 of 23386 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.23%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.473500
a=0.000000 b=1.000000 c=22.473500
From vast_summary.log: estimated ref. image limiting mag.: -7.79
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.68
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23386 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0031 to 359.9999 deg, Dec +48.2162 to +59.2586 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0031 to 359.9999 deg, Dec 48.2162 to 59.2586 deg
Loaded 153985 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 53 out of 58 total matches.
Matched with Tycho-2 58 out of 23386 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (aperture=6.2)
Read 23366 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0031 to 360.0000 deg, Dec +48.2161 to +59.2689 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0031 to 360.0000 deg, Dec 48.2161 to 59.2689 deg
Loaded 154106 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 50 out of 55 total matches.
Matched with Tycho-2 55 out of 23366 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
2.3 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Limiting magnitude estimates:
14.7 mag. Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
14.7 mag. Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
12.8 mag. fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
13.0 mag. fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DIIhyVtZ1r (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1910, bad_region=5051, passed=23386
Got 23386 stars (including 16726 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 23386 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.0'
Seting catalog search parameters based on the expected field of view 927.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012875 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010300 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9996 through 0 to 14.8812, gap 14.8812 to 344.9996
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 325 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 241 matched stars entering correct_measured_positions(), 168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 4908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.09"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9814 through 0 to 14.9033, gap 14.9033 to 344.9814
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 397 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 328 matched stars entering correct_measured_positions(), 4961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.99"
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 6645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.24"
Excluding outliers - 325 stars left (next iteration limit 256)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits N_match=325 sigma_overall_arcsec=11.131 sigma_q1_arcsec=25.602 sigma_q2_arcsec=32.104 sigma_q3_arcsec=8.250 sigma_q4_arcsec=9.745 n_q1=41 n_q2=23 n_q3=116 n_q4=145 worst_quadrant_to_overall_ratio=2.884
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.i7zfPQ5I5d (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1872, bad_region=4985, passed=23366
Got 23366 stars (including 16797 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 23366 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.1'
Seting catalog search parameters based on the expected field of view 927.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012876 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010301 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0112 through 0 to 14.8810, gap 14.8810 to 345.0112
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 239 matched stars entering correct_measured_positions(), 165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 231 matched stars entering correct_measured_positions(), 4693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9936 through 0 to 14.9023, gap 14.9023 to 344.9936
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 397 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 321 matched stars entering correct_measured_positions(), 4741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.79"
Accuracy estimation diagnostic: 315 matched stars entering correct_measured_positions(), 6313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.43"
Excluding outliers - 315 stars left (next iteration limit 254)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits N_match=315 sigma_overall_arcsec=10.449 sigma_q1_arcsec=28.329 sigma_q2_arcsec=30.359 sigma_q3_arcsec=8.438 sigma_q4_arcsec=7.803 n_q1=34 n_q2=19 n_q3=120 n_q4=142 worst_quadrant_to_overall_ratio=2.905
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1CkBazGYVX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=142, bad_region=954, passed=3444
Got 3444 stars (including 2383 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat
util/solve_plate_with_UCAC5 got 3444 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
RA wraps around 0/360 boundary: field RA 344.6889 through 0 to 14.6165, gap 14.6165 to 344.6889
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.4 to 59.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 2543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.6863 through 0 to 14.6173, gap 14.6173 to 344.6863
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.4 to 59.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 2542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 2542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits N_match=963 sigma_overall_arcsec=0.613 sigma_q1_arcsec=0.675 sigma_q2_arcsec=0.580 sigma_q3_arcsec=0.696 sigma_q4_arcsec=0.631 n_q1=188 n_q2=275 n_q3=229 n_q4=271 worst_quadrant_to_overall_ratio=1.135
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.aEdD8Wj29y (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=227, bad_region=1144, passed=4767
Got 4767 stars (including 3446 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat
util/solve_plate_with_UCAC5 got 4767 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
RA wraps around 0/360 boundary: field RA 344.6936 through 0 to 14.6159, gap 14.6159 to 344.6936
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 972 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(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 3613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.6910 through 0 to 14.6169, gap 14.6169 to 344.6910
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 972 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(), 3616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 3616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits N_match=972 sigma_overall_arcsec=0.609 sigma_q1_arcsec=0.644 sigma_q2_arcsec=0.572 sigma_q3_arcsec=0.696 sigma_q4_arcsec=0.523 n_q1=145 n_q2=221 n_q3=338 n_q4=268 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits sigma_overall=11.131 worst_q_ratio=2.884
ref2=Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits sigma_overall=10.449 worst_q_ratio=2.905
new1=fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits sigma_overall=0.613 worst_q_ratio=1.135
new2=fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits sigma_overall=0.609 worst_q_ratio=1.142
reference average sigma_overall=10.79 worst_q_ratio=2.8945
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006_astrometric_residuals.png (325 matched stars from wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.67 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007_astrometric_residuals.png (315 matched stars from wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.55 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112_astrometric_residuals.png (963 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.58 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113_astrometric_residuals.png (972 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05724_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 05724_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:09:36.53 +51:34:00.7 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-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Image size: 927.0'x616.4' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:01.466 +54:00:23.28 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
Image size: 939.0'x624.3' 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: 23:59:25.538 +54:00:50.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 23:59:25.538 +54:00:50.88
Angular distance between the image centers 0.0883 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Image size: 939.0'x624.3' 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: 23:59:29.589 +54:01:19.49 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 23:59:29.589 +54:01:19.49
Angular distance between the image centers 0.0796 deg.
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# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:25.538 +54:00:50.88
Second-epoch second image center 23:59:29.589 +54:01:19.49
Angular distance between the image centers 0.01271 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits &> /tmp/tmp.pmjR46sN6h
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits &> /tmp/tmp.xIVPtLgS8K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits &> /tmp/tmp.Ayu3OVyFmO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits &> /tmp/tmp.b5atzQm9T4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 167282 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +48.1859 to +59.2631 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0000 to 360.0000 deg, Dec 48.1859 to 59.2631 deg
Loaded 154477 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 105 out of 150 total matches.
Matched with Tycho-2 150 out of 167282 detected stars.
ERROR: only 105 of 167282 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.06%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.702700
a=0.000000 b=1.000000 c=20.702700
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 167282 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +48.1859 to +59.2631 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0000 to 360.0000 deg, Dec 48.1859 to 59.2631 deg
Loaded 154477 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 105 out of 150 total matches.
Matched with Tycho-2 150 out of 167282 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (aperture=4.7)
Read 165704 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +48.1861 to +59.2705 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0000 to 360.0000 deg, Dec 48.1861 to 59.2705 deg
Loaded 154563 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 102 out of 145 total matches.
Matched with Tycho-2 145 out of 165704 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.2 pix Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
2.1 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Limiting magnitude estimates:
13.3 mag. Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
13.2 mag. Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
11.5 mag. fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
11.7 mag. fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
All-image limiting magnitude estimate: 11.5 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.pmjR46sN6h (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=20826, bad_region=21165, passed=167247
Got 167247 stars (including 127895 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 167247 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.0'
Seting catalog search parameters based on the expected field of view 927.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012875 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010300 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9631 through 0 to 14.9764, gap 14.9764 to 344.9631
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 318 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 216 matched stars entering correct_measured_positions(), 35553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9503 through 0 to 14.9983, gap 14.9983 to 344.9503
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 395 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 320 matched stars entering correct_measured_positions(), 35597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.35"
Accuracy estimation diagnostic: 315 matched stars entering correct_measured_positions(), 52070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.79"
Excluding outliers - 315 stars left (next iteration limit 237)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits N_match=315 sigma_overall_arcsec=8.955 sigma_q1_arcsec=30.923 sigma_q2_arcsec=19.444 sigma_q3_arcsec=6.520 sigma_q4_arcsec=8.008 n_q1=39 n_q2=21 n_q3=117 n_q4=138 worst_quadrant_to_overall_ratio=3.453
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xIVPtLgS8K (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=39, blended=20515, bad_region=20705, passed=165665
Got 165665 stars (including 126839 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 165665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.1'
Seting catalog search parameters based on the expected field of view 927.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012876 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010301 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9474 through 0 to 14.9341, gap 14.9341 to 344.9474
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 326 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 225 matched stars entering correct_measured_positions(), 37244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9404 through 0 to 14.9637, gap 14.9637 to 344.9404
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 400 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 37289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.64"
Accuracy estimation diagnostic: 317 matched stars entering correct_measured_positions(), 52373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.41"
Excluding outliers - 317 stars left (next iteration limit 247)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits N_match=317 sigma_overall_arcsec=8.596 sigma_q1_arcsec=27.471 sigma_q2_arcsec=23.969 sigma_q3_arcsec=6.420 sigma_q4_arcsec=8.419 n_q1=37 n_q2=20 n_q3=128 n_q4=132 worst_quadrant_to_overall_ratio=3.196
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Ayu3OVyFmO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1495, bad_region=8948, passed=37144
Got 37144 stars (including 26998 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat
util/solve_plate_with_UCAC5 got 37144 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
RA wraps around 0/360 boundary: field RA 344.6890 through 0 to 14.6164, gap 14.6164 to 344.6890
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 28747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.6859 through 0 to 14.6172, gap 14.6172 to 344.6859
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 28748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 28748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits N_match=954 sigma_overall_arcsec=0.585 sigma_q1_arcsec=0.648 sigma_q2_arcsec=0.551 sigma_q3_arcsec=0.681 sigma_q4_arcsec=0.606 n_q1=206 n_q2=271 n_q3=198 n_q4=279 worst_quadrant_to_overall_ratio=1.164
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.b5atzQm9T4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2342, bad_region=10530, passed=48868
Got 48868 stars (including 36363 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat
util/solve_plate_with_UCAC5 got 48868 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
RA wraps around 0/360 boundary: field RA 344.6936 through 0 to 14.6555, gap 14.6555 to 344.6936
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 38675 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.6910 through 0 to 14.6565, gap 14.6565 to 344.6910
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 38672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 38670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits N_match=970 sigma_overall_arcsec=0.589 sigma_q1_arcsec=0.639 sigma_q2_arcsec=0.537 sigma_q3_arcsec=0.708 sigma_q4_arcsec=0.505 n_q1=167 n_q2=225 n_q3=291 n_q4=287 worst_quadrant_to_overall_ratio=1.202
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-42-34_20.00sec_5.00C_LIGHT_0112.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_Cas-04-Q2b1x1_234724_TTUQ2b1x1_547564_KrMidM8W/wcs_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:40:53.01 +58:05:25.0: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:11.83 +50:30:00.5: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:21:39.71 +55:23:07.1: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:38.39 +57:26:54.4: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:55:25.78 +50:00:50.5: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:23.31 +55:49:11.2: 13.58 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:22:45.25 +50:48:14.6: 13.65 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:26:10.87 +57:09:01.8: 12.95 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:42.12 +53:02:30.1: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:47.70 +56:39:17.8: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:40:53.01 +58:05:25.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:55:25.78 +50:00:50.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:23.31 +55:49:11.2: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:11.83 +50:30:00.5: 13.34 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:22:45.25 +50:48:14.6: 13.42 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:10.87 +57:09:01.8: 13.29 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:21:39.71 +55:23:07.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:42.12 +53:02:30.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:38.39 +57:26:54.4: 13.39 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.58 +/- 0.32
Forced photometry reference-image weighted average: 13.34 +/- 0.35
Forced photometry reference-image weighted average: 13.54 +/- 0.23
Forced photometry reference-image weighted average: 13.04 +/- 0.15
Forced photometry filter KEPT candidate at 00:30:23.31 +55:49:11.2: ref_mag=13.58 +/- 0.32 new_mean_mag=10.9384 delta=2.64 (need > 0.90)
Forced photometry filter KEPT candidate at 23:58:11.83 +50:30:00.5: ref_mag=13.34 +/- 0.35 new_mean_mag=11.0840 delta=2.26 (need > 0.90)
Forced photometry filter KEPT candidate at 00:22:45.25 +50:48:14.6: ref_mag=13.54 +/- 0.23 new_mean_mag=11.1516 delta=2.39 (need > 0.90)
Forced photometry filter KEPT candidate at 00:26:10.87 +57:09:01.8: ref_mag=13.04 +/- 0.15 new_mean_mag=11.0707 delta=1.96 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:47.70 +56:39:17.8: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:02:42.03 +50:03:44.0: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:02:42.03 +50:03:44.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:48.95 +50:53:17.5: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:23.03 +50:57:10.1: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:54:48.95 +50:53:17.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:23.03 +50:57:10.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:52.71 +51:31:14.3: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:52.71 +51:31:14.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:09.55 +50:24:08.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:09.55 +50:24:08.7: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:24:30.34 +52:14:19.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:10.81 +56:29:42.5: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:10.81 +56:29:42.5: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:24:30.34 +52:14:19.4: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:34.61 +50:02:30.0: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:34.61 +50:02:30.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:41.93 +57:00:51.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:14:07.25 +51:33:29.2: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:41.93 +57:00:51.0: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:14:07.25 +51:33:29.2: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:23.70 +55:26:50.8: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:23.70 +55:26:50.8: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:13:17.61 +50:25:36.1: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:13:17.61 +50:25:36.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:12:08.66 +50:38:18.9: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:12:08.66 +50:38:18.9: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:11:16.72 +50:50:57.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:06:29.52 +50:07:47.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:11:16.72 +50:50:57.7: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:06:29.52 +50:07:47.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:04:13.36 +51:32:55.3: 13.11 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:32.89 +57:40:49.0: 13.31 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:04:13.36 +51:32:55.3: 13.08 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.14
Forced photometry filter KEPT candidate at 00:04:13.36 +51:32:55.3: ref_mag=13.10 +/- 0.14 new_mean_mag=11.0647 delta=2.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:32.89 +57:40:49.0: 13.31 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.31 +/- 0.27
Forced photometry filter KEPT candidate at 00:19:32.89 +57:40:49.0: ref_mag=13.31 +/- 0.27 new_mean_mag=10.9434 delta=2.37 (need > 0.90)
Adding exclusion_list_local.txt__out189883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190179.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 43s
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: 18s
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Considering the candidate 189883_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189883_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
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Considering the candidate 189884_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 189884_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 23:58:49.91 +53:25:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189885_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189885_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
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Considering the candidate 189887_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189887_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
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Considering the candidate 189889_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189889_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
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Considering the candidate 189893_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189893_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
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Considering the candidate 189897_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189897_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
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Considering the candidate 189898_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189898_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
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Considering the candidate 189905_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189905_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
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Considering the candidate 189910_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189910_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
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Considering the candidate 189913_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189913_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189916_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189916_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189918_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189918_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189919_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189919_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189920_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189920_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189922_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189922_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189923_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189923_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189926_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189926_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189928_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 189928_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:14:48.87 +51:48:53.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189931_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 189931_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:00:53.05 +49:57:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189984_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 189984_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190001_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 190001_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:20:50.24 +54:00:26.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190002_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 190002_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:18:59.59 +53:18:06.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190009_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 190009_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:10:46.81 +49:57:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190019_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 190019_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190035_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 190035_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190064_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 190064_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:10:01.44 +50:48:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190084_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 190084_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:23:03.58 +55:45:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190094_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 190094_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190095_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 190095_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190129_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 190129_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190130_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 190130_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:13:37.61 +56:24:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190131_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 190131_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190138_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 190138_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190176_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 190176_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190179_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
Preparing report for the candidate 190179_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35911_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113
The candidate 35911_fd_Cas-04-Q2b1x1_2026-07-10_23-43-34_20.00sec_4.90C_LIGHT_0113 did not pass the final checks
**** FOUND 00:09:36.49 +51:34:01.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 64s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:21:39.71 +55:23:07.1
00:27:38.39 +57:26:54.4
00:30:23.31 +55:49:11.2
00:17:42.12 +53:02:30.1
00:22:45.25 +50:48:14.6
23:58:11.83 +50:30:00.5
00:26:10.87 +57:09:01.8
23:55:25.78 +50:00:50.5
23:40:53.01 +58:05:25.0
00:28:47.70 +56:39:17.8
00:02:42.03 +50:03:44.0
23:54:48.95 +50:53:17.5
00:07:23.03 +50:57:10.1
00:19:52.71 +51:31:14.3
23:57:09.55 +50:24:08.7
00:24:30.34 +52:14:19.4
00:28:10.81 +56:29:42.5
00:19:34.61 +50:02:30.0
00:14:07.25 +51:33:29.2
00:28:41.93 +57:00:51.0
00:25:23.70 +55:26:50.8
00:13:17.61 +50:25:36.1
00:12:08.66 +50:38:18.9
00:11:16.72 +50:50:57.7
00:06:29.52 +50:07:47.8
00:04:13.36 +51:32:55.3
00:19:32.89 +57:40:49.0
########### Completed Cas-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
00:21:39.71 +55:23:07.1
00:27:38.39 +57:26:54.4
00:30:23.31 +55:49:11.2
00:17:42.12 +53:02:30.1
00:22:45.25 +50:48:14.6
23:58:11.83 +50:30:00.5
00:26:10.87 +57:09:01.8
23:55:25.78 +50:00:50.5
23:40:53.01 +58:05:25.0
00:28:47.70 +56:39:17.8
00:02:42.03 +50:03:44.0
23:54:48.95 +50:53:17.5
00:07:23.03 +50:57:10.1
00:19:52.71 +51:31:14.3
23:57:09.55 +50:24:08.7
00:24:30.34 +52:14:19.4
00:28:10.81 +56:29:42.5
00:19:34.61 +50:02:30.0
00:14:07.25 +51:33:29.2
00:28:41.93 +57:00:51.0
00:25:23.70 +55:26:50.8
00:13:17.61 +50:25:36.1
00:12:08.66 +50:38:18.9
00:11:16.72 +50:50:57.7
00:06:29.52 +50:07:47.8
00:04:13.36 +51:32:55.3
00:19:32.89 +57:40:49.0
###################################################################################
00:21:39.71 +55:23:07.1 -- not an asteroid (will add it to exclusion list)
00:27:38.39 +57:26:54.4 -- not an asteroid (will add it to exclusion list)
00:30:23.31 +55:49:11.2 -- not an asteroid (will add it to exclusion list)
00:17:42.12 +53:02:30.1 -- not an asteroid (will add it to exclusion list)
00:22:45.25 +50:48:14.6 -- not an asteroid (will add it to exclusion list)
23:58:11.83 +50:30:00.5 -- not an asteroid (will add it to exclusion list)
00:26:10.87 +57:09:01.8 -- not an asteroid (will add it to exclusion list)
23:55:25.78 +50:00:50.5 -- not an asteroid (will add it to exclusion list)
23:40:53.01 +58:05:25.0 -- not an asteroid (will add it to exclusion list)
00:28:47.70 +56:39:17.8 -- not an asteroid (will add it to exclusion list)
00:02:42.03 +50:03:44.0 -- not an asteroid (will add it to exclusion list)
23:54:48.95 +50:53:17.5 -- not an asteroid (will add it to exclusion list)
00:07:23.03 +50:57:10.1 -- not an asteroid (will add it to exclusion list)
00:19:52.71 +51:31:14.3 -- not an asteroid (will add it to exclusion list)
23:57:09.55 +50:24:08.7 -- not an asteroid (will add it to exclusion list)
00:24:30.34 +52:14:19.4 -- not an asteroid (will add it to exclusion list)
00:28:10.81 +56:29:42.5 -- not an asteroid (will add it to exclusion list)
00:19:34.61 +50:02:30.0 -- not an asteroid (will add it to exclusion list)
00:14:07.25 +51:33:29.2 -- not an asteroid (will add it to exclusion list)
00:28:41.93 +57:00:51.0 -- not an asteroid (will add it to exclusion list)
00:25:23.70 +55:26:50.8 -- not an asteroid (will add it to exclusion list)
00:13:17.61 +50:25:36.1 -- not an asteroid (will add it to exclusion list)
00:12:08.66 +50:38:18.9 -- not an asteroid (will add it to exclusion list)
00:11:16.72 +50:50:57.7 -- not an asteroid (will add it to exclusion list)
00:06:29.52 +50:07:47.8 -- not an asteroid (will add it to exclusion list)
00:04:13.36 +51:32:55.3 -- not an asteroid (will add it to exclusion list)
00:19:32.89 +57:40:49.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:02:42.03 +50:03:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:13.36 +51:32:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:29.52 +50:07:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:23.03 +50:57:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:16.72 +50:50:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:08.66 +50:38:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:17.61 +50:25:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:07.25 +51:33:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:42.12 +53:02:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:32.89 +57:40:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:34.61 +50:02:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:52.71 +51:31:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:39.71 +55:23:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:45.25 +50:48:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:30.34 +52:14:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:23.70 +55:26:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:10.87 +57:09:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:38.39 +57:26:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:10.81 +56:29:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:41.93 +57:00:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:47.70 +56:39:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:23.31 +55:49:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:53.01 +58:05:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:48.95 +50:53:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:25.78 +50:00:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:09.55 +50:24:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:11.83 +50:30:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:02:42.03 +50:03:44.0 -- not a known variable star
00:04:13.36 +51:32:55.3 -- not a known variable star
00:06:29.52 +50:07:47.8 -- not a known variable star
00:07:23.03 +50:57:10.1 -- not a known variable star
00:11:16.72 +50:50:57.7 -- not a known variable star
00:12:08.66 +50:38:18.9 -- not a known variable star
00:13:17.61 +50:25:36.1 -- not a known variable star
00:14:07.25 +51:33:29.2 -- not a known variable star
00:17:42.12 +53:02:30.1 -- not a known variable star
00:19:32.89 +57:40:49.0 -- a known variable star
00:19:34.61 +50:02:30.0 -- not a known variable star
00:19:52.71 +51:31:14.3 -- not a known variable star
00:21:39.71 +55:23:07.1 -- not a known variable star
00:22:45.25 +50:48:14.6 -- not a known variable star
00:24:30.34 +52:14:19.4 -- not a known variable star
00:25:23.70 +55:26:50.8 -- not a known variable star
00:26:10.87 +57:09:01.8 -- not a known variable star
00:27:38.39 +57:26:54.4 -- not a known variable star
00:28:10.81 +56:29:42.5 -- not a known variable star
00:28:41.93 +57:00:51.0 -- a known variable star
00:28:47.70 +56:39:17.8 -- not a known variable star
00:30:23.31 +55:49:11.2 -- a known variable star
23:40:53.01 +58:05:25.0 -- not a known variable star
23:54:48.95 +50:53:17.5 -- not a known variable star
23:55:25.78 +50:00:50.5 -- not a known variable star
23:57:09.55 +50:24:08.7 -- not a known variable star
23:58:11.83 +50:30:00.5 -- not a known variable star
Found 24 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
27 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
00:02:42.03 +50:03:44.0
00:04:13.36 +51:32:55.3
00:06:29.52 +50:07:47.8
00:07:23.03 +50:57:10.1
00:11:16.72 +50:50:57.7
00:12:08.66 +50:38:18.9
00:13:17.61 +50:25:36.1
00:14:07.25 +51:33:29.2
00:17:42.12 +53:02:30.1
00:19:32.89 +57:40:49.0
00:19:34.61 +50:02:30.0
00:19:52.71 +51:31:14.3
00:21:39.71 +55:23:07.1
00:22:45.25 +50:48:14.6
00:24:30.34 +52:14:19.4
00:25:23.70 +55:26:50.8
00:26:10.87 +57:09:01.8
00:27:38.39 +57:26:54.4
00:28:10.81 +56:29:42.5
00:28:41.93 +57:00:51.0
00:28:47.70 +56:39:17.8
00:30:23.31 +55:49:11.2
23:40:53.01 +58:05:25.0
23:54:48.95 +50:53:17.5
23:55:25.78 +50:00:50.5
23:57:09.55 +50:24:08.7
23:58:11.83 +50:30:00.5
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461232.69634522 -observatory V36
07:29:59.64 +17:06:26.7 Mercury (5.3mag)
10:15:10.85 +12:18:42.6 Venus (-4.1mag)
04:26:40.57 +21:31:29.1 Mars (1.3mag)
08:17:26.60 +20:09:03.7 Jupiter (-1.8mag)
00:55:56.35 +03:20:47.7 Saturn (0.7mag)
04:07:23.69 +20:45:29.5 Uranus (5.8mag)
00:17:01.21 +00:20:36.5 Neptune (7.7mag)
20:30:50.28 -23:18:22.9 Pluto (14.4mag)
04:01:48.40 +25:01:49.8 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Jul 11 00:53 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461232.69634522:
08:17:23.22 +20:09:15.8 Io (6.1mag)
08:17:38.01 +20:08:21.4 Europa (6.3mag)
08:17:42.26 +20:08:03.8 Ganymede (5.6mag)
08:17:49.93 +20:07:35.4 Callisto (6.8mag)
08:15:55.73 +19:53:34.4 Himalia (15.7mag)
08:17:30.64 +20:08:48.8 Thebe (16.6mag)
08:15:16.86 +19:57:51.9 Elara (17.6mag)
08:21:00.40 +20:02:46.5 Pasiphae (17.8mag)
08:22:21.55 +20:14:15.8 Carme (19.0mag)
00:55:48.91 +03:20:29.4 Titan (8.5mag)
00:55:54.29 +03:20:36.7 Rhea (9.8mag)
00:55:24.66 +03:19:46.9 Iapetus (11.2mag)
00:56:02.28 +03:21:12.3 Hyperion (14.5mag)
00:55:55.96 +03:17:54.1 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 11 00:53 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461232.69634522:
17:47:58.00 -32:49:57.6 JWST
18:05:33.71 +32:35:40.9 Chandra
08:51:16.33 -49:48:15.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 11 00:53 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461232.69634522 -observatory V36
02:37:28.26 +14:31:44.5 17.9mag P/1996 R2 (Lagerkvist)
18:17:17.52 -34:23:11.7 13.7mag P/2010 H2 (Vales)
06:26:31.17 -68:09:10.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:01:05.99 +32:27:40.6 17.6mag C/2017 K2 (PANSTARRS)
17:02:52.66 +16:02:37.3 18.0mag C/2021 G2 (ATLAS)
01:52:36.77 +09:53:20.2 15.4mag P/2021 N1 (ZTF)
22:59:01.68 +32:17:03.7 17.3mag C/2022 E2 (ATLAS)
06:13:21.81 +26:55:08.2 16.7mag C/2022 N2 (PANSTARRS)
09:56:14.95 +29:44:35.8 16.8mag C/2022 QE78 (ATLAS)
09:10:16.74 +05:00:56.4 17.8mag C/2022 R6 (PANSTARRS)
18:06:42.20 +21:15:43.2 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:30.09 -11:24:24.9 17.7mag P/2023 B1 (PANSTARRS)
21:48:13.53 +67:36:58.3 17.8mag C/2023 H5 (Lemmon)
16:29:13.07 -10:10:00.5 13.9mag C/2023 R1 (PANSTARRS)
08:02:06.54 +65:45:13.4 17.9mag C/2024 A1 (ATLAS)
07:33:55.28 +30:02:48.3 14.6mag C/2024 E1 (Wierzchos)
15:15:55.02 +15:21:03.9 17.6mag C/2024 G6 (ATLAS)
19:40:14.47 +39:33:31.9 13.8mag C/2024 J3 (ATLAS)
21:46:42.95 +46:07:50.6 17.8mag C/2024 R4 (PANSTARRS)
04:50:26.21 -13:45:25.9 15.7mag C/2024 T5 (ATLAS)
06:35:16.37 +28:55:44.6 18.0mag C/2025 J1 (Borisov)
07:14:55.93 -12:57:50.2 16.5mag C/2025 R3 (PANSTARRS)
09:57:04.02 +22:24:03.9 17.6mag C/2025 V2 (Rankin)
12:44:53.81 +03:54:07.5 17.1mag C/2025 Y1 (ATLAS)
16:49:34.32 +79:08:18.9 17.3mag C/2026 A2 (Bok)
02:47:10.69 +45:16:35.0 16.7mag C/2026 B2 (Sun-Gao)
11:26:02.72 +04:41:43.3 17.0mag A/2026 E1
21:20:22.95 -15:22:31.1 7.2mag 10P/Tempel
11:13:50.94 -01:55:23.1 16.1mag 29P/Schwassmann-Wachmann
04:01:23.42 +29:38:42.6 17.9mag 47P/Ashbrook-Jackson
10:09:50.39 +13:44:34.0 17.0mag 63P/Wild
00:48:43.99 -05:04:58.2 15.5mag 65P/Gunn
08:29:35.27 +34:10:43.5 18.0mag 76P/West-Kohoutek-Ikemura
04:29:26.42 +20:13:23.5 13.7mag 78P/Gehrels
02:23:42.40 +10:43:36.7 16.2mag 88P/Howell
06:38:02.85 +30:29:09.6 15.7mag 93P/Lovas
04:23:44.08 +31:09:33.2 16.8mag 114P/Wiseman-Skiff
08:10:45.39 +30:36:37.4 15.2mag 123P/West-Hartley
10:49:42.20 +00:50:34.7 16.8mag 124P/Mrkos
04:53:05.10 +20:50:15.0 16.2mag 128P/Shoemaker-Holt
05:37:50.92 +19:42:28.5 17.8mag 131P/Mueller
00:01:46.75 +02:58:07.3 17.9mag 139P/Vaisala-Oterma
07:16:41.10 +16:50:20.5 15.6mag 141P-D/Machholz
03:17:12.48 -21:02:04.9 15.4mag 161P/Hartley-IRAS
05:36:06.02 +34:07:55.4 15.3mag 162P/SidingSpring
19:02:21.60 +15:35:53.5 14.7mag 169P/NEAT
01:43:03.10 +07:41:40.4 17.7mag 220P/McNaught
16:35:51.17 -08:25:05.2 17.0mag 235P/LINEAR
08:47:03.98 +33:13:19.8 17.9mag 240P/NEAT
20:41:50.22 -49:45:23.5 17.8mag 259P/Garradd
02:01:39.99 +12:29:23.0 15.7mag 260P/McNaught
05:39:46.95 +36:54:41.6 17.4mag 295P/LINEAR
15:06:34.01 +05:58:56.1 17.6mag 391P/Kowalski
08:35:21.59 +19:38:33.8 17.9mag 450P/LONEOS
07:53:05.56 +39:08:46.6 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 11 00:53 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 11 00:53 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 11 00:53 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:43:56.471 -07:01:02.12 AT 2026syg 2026-06-27.41 22.6378
22:44:27.893 -09:14:49.58 AT 2026syf 2026-06-27.41 22.7315
23:02:17.769 -08:54:25.49 AT 2026sye 2026-06-27.42 21.7254
20:14:56.619 -18:30:02.61 AT 2026syd 2026-06-27.29 22.2007
20:49:57.648 -11:42:25.46 AT 2026syc 2026-06-27.30 22.962
21:15:07.018 -10:44:08.34 AT 2026syb 2026-06-27.34 22.1382
21:45:53.908 -10:06:22.31 AT 2026sya 2026-06-27.33 22.2361
21:28:25.130 -19:21:16.37 AT 2026sxz 2026-06-27.33 22.3064
22:56:47.457 -11:33:53.05 AT 2026sxy 2026-06-27.41 22.3592
23:00:56.153 -09:26:33.73 AT 2026sxx 2026-06-27.42 22.4667
23:07:22.508 -08:39:16.38 AT 2026sxw 2026-06-27.42 23.0272
23:22:51.227 -12:58:53.91 AT 2026sxv 2026-06-27.42 22.3827
23:16:07.929 -14:23:36.62 AT 2026sxu 2026-06-27.41 23.2261
23:04:02.238 -12:22:56.76 AT 2026sxt 2026-06-27.39 22.0508
21:10:17.846 -12:44:21.11 AT 2026sxs 2026-06-27.37 21.8392
19:55:22.564 -17:06:27.50 AT 2026sxr 2026-06-27.29 21.3456
23:00:02.745 -08:30:24.16 AT 2026sxq 2026-06-27.42 22.8616
21:14:05.963 -13:23:09.24 AT 2026sxp 2026-06-27.34 22.6391
21:10:37.720 -17:10:12.78 AT 2026sxo 2026-06-27.34 23.0493
21:07:16.782 -18:35:52.19 AT 2026sxn 2026-06-27.34 22.8686
-rw-r--r-- 1 apache apache 30K Jul 11 00:53 tns_transients_list.txt
