This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.82 01:26:37.00 +63:57:53.6
126.78093 1.35635 galactic Cas Second-epoch detections are separated by 1.9" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:26:37.00 +63:57:53.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:37.00 +63:57:53.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:37.00 +63:57:53.6: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 26 37.00 +63 57 53.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461170.9112,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260510.4112 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.82 01:07:05.11 +64:43:58.6
124.60150 1.91193 galactic Cas Second-epoch detections are separated by 2.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:05.11 +64:43:58.6 (user input) | T | P | (position from user input) J-Ks=0.523+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:05.11 +64:43:58.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:05.11 +64:43:58.6: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 07 05.11 +64 43 58.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461170.9112,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260510.4112 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.78 01:50:46.59 +58:00:39.0
130.74597 -3.95783 galactic Per Second-epoch detections are separated by 2.4" and 2.7 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 J027.6849+58.0117 | 01:50:46.59 +58:00:39.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:46.59 +58:00:39.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:46.59 +58:00:39.0: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 50 46.59 +58 00 39.0 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J027.6849+58.0117,2461170.9112,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J027.6849+58.0117 20260510.4112 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.84 01:58:54.80 +58:10:52.1
131.74928 -3.53078 galactic Cas Second-epoch detections are separated by 4.1" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:58:54.80 +58:10:52.1 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:54.80 +58:10:52.1: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:54.80 +58:10:52.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 58 54.80 +58 10 52.1 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
target,2461170.9112,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260510.4112 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.76 02:01:35.90 +64:25:06.5
130.41668 2.57111 galactic Cas Second-epoch detections are separated by 0.9" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:01:35.90 +64:25:06.5 (user input) | T | P | (position from user input) J-Ks=0.537+/-0.117 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:35.90 +64:25:06.5: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:35.90 +64:25:06.5: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 02 01 35.90 +64 25 06.5 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461170.9112,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260510.4112 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.63 01:14:01.35 +57:40:46.4
125.95896 -5.05939 galactic Cas Second-epoch detections are separated by 3.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:14:01.35 +57:40:46.4 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:01.35 +57:40:46.4: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:01.35 +57:40:46.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 14 01.35 +57 40 46.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461170.9112,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260510.4112 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.64 01:07:35.02 +57:33:10.4
125.10540 -5.25071 galactic Cas Second-epoch detections are separated by 1.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:35.02 +57:33:10.4 (user input) | T | P | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.856+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:35.02 +57:33:10.4: 11.95 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:35.02 +57:33:10.4: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 07 35.02 +57 33 10.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461170.9112,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260510.4112 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.70 01:11:24.95 +64:28:44.6
125.08246 1.69076 galactic Cas Second-epoch detections are separated by 2.5" and 2.3 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 524958154490117760 | 01:11:22.23 +64:28:48.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:24.95 +64:28:44.6: 12.22 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:24.95 +64:28:44.6: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 11 24.95 +64 28 44.6 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 524958154490117760,2461170.9112,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524958154490117760 20260510.4112 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.44 01:57:36.50 +58:59:34.5
131.37635 -2.78967 galactic Cas Second-epoch detections are separated by 1.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:57:36.50 +58:59:34.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:36.50 +58:59:34.5: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:36.50 +58:59:34.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 57 36.50 +58 59 34.5 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
target,2461170.9112,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260510.4112 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.68 01:33:01.46 +59:16:32.1
128.23017 -3.16769 galactic Cas Second-epoch detections are separated by 4.9" and 3.7 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 | ASASSN-V J013303.78+591550.3 | 01:33:03.78 +59:15:50.3 (Gaia DR3) | SRS (local) | 16.088000000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:01.46 +59:16:32.1: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:01.46 +59:16:32.1: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 33 01.46 +59 16 32.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013303.78+591550.3,2461170.9112,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013303.78+591550.3 20260510.4112 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.34 01:22:43.71 +64:18:30.2
126.31608 1.64244 galactic Cas Second-epoch detections are separated by 4.0" and 3.2 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 512802705549896576 | 01:22:42.51 +64:18:38.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:43.71 +64:18:30.2: 11.67 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:43.71 +64:18:30.2: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 22 43.71 +64 18 30.2 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 512802705549896576,2461170.9112,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512802705549896576 20260510.4112 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.27 01:06:17.51 +65:05:27.9
124.49627 2.26446 galactic Cas Second-epoch detections are separated by 7.5" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 525049998070146048 | 01:06:13.92 +65:05:30.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:17.51 +65:05:27.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:17.51 +65:05:27.9: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 06 17.51 +65 05 27.9 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 525049998070146048,2461170.9112,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 525049998070146048 20260510.4112 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.40 01:13:46.44 +57:24:46.4
125.94903 -5.32795 galactic Cas Second-epoch detections are separated by 2.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:13:46.44 +57:24:46.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:46.44 +57:24:46.4: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:46.44 +57:24:46.4: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 13 46.44 +57 24 46.4 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
target,2461170.9112,10.40,0.05,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
target 20260510.4112 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 05 10.4112 2461170.9112 10.36 01:57:52.26 +63:48:34.5
130.18307 1.87704 galactic Cas Second-epoch detections are separated by 0.8" and 2.6 pix
The object was found in VSX14" ASASSN-V J015753.42+634846.1
Type: SR
# Max. Min./Amp. JD0 Period
13.590 V 13.970 V 2458299.91990 150.638151100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:52.26 +63:48:34.5: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:52.26 +63:48:34.5: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 57 52.26 +63 48 34.5 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
ASASSN-V J015753.42+634846.1,2461170.9112,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J015753.42+634846.1 20260510.4112 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.38 01:36:26.15 +64:32:07.7
127.74649 2.08518 galactic Cas Second-epoch detections are separated by 1.9" and 3.1 pix
The object was found in VSX16" Gaia DR3 512961550618235392
Type: RS
# Max. Min./Amp. JD0 Period
13.970 G 14.110 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:26.15 +64:32:07.7: 12.71 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:26.15 +64:32:07.7: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 36 26.15 +64 32 07.7 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 512961550618235392,2461170.9112,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512961550618235392 20260510.4112 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 9.59 01:15:16.86 +57:28:05.4
126.14684 -5.25467 galactic Cas Second-epoch detections are separated by 1.6" and 2.6 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 413443898501160704 | 01:15:18.56 +57:27:47.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.238+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:16.86 +57:28:05.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:16.86 +57:28:05.4: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 15 16.86 +57 28 05.4 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413443898501160704,2461170.9112,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413443898501160704 20260510.4112 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.52 01:26:35.81 +57:57:40.7
127.59663 -4.59165 galactic Cas Second-epoch detections are separated by 0.7" and 2.7 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 J021.6500+57.9729 | 01:26:33.58 +57:57:55.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:35.81 +57:57:40.7: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:35.81 +57:57:40.7: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 26 35.81 +57 57 40.7 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 J021.6500+57.9729,2461170.9112,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.6500+57.9729 20260510.4112 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.55 01:54:53.15 +58:16:50.2
131.21014 -3.56769 galactic Cas Second-epoch detections are separated by 4.3" and 2.2 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 J028.7238+58.2897 | 01:54:53.15 +58:16:50.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:53.15 +58:16:50.2: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:53.15 +58:16:50.2: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 54 53.15 +58 16 50.2 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J028.7238+58.2897,2461170.9112,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J028.7238+58.2897 20260510.4112 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.62 01:14:58.20 +60:30:25.1
125.82657 -2.23245 galactic Cas Second-epoch detections are separated by 4.0" and 2.4 pix
The object was found in VSX 5" Mis V1361
Type: EA
# Max. Min./Amp. JD0 Period
13.551 r Y 0.490 r 2458282.97450 1.603348400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:58.20 +60:30:25.1: 12.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:58.20 +60:30:25.1: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 14 58.20 +60 30 25.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1361,2461170.9112,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V1361 20260510.4112 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.61 01:55:52.81 +64:15:31.8
129.85923 2.25727 galactic Cas Second-epoch detections are separated by 4.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:55:52.81 +64:15:31.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:52.81 +64:15:31.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:52.81 +64:15:31.8: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 55 52.81 +64 15 31.8 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461170.9112,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260510.4112 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.70 02:16:02.74 +60:37:00.8
133.13018 -0.56865 galactic Cas Second-epoch detections are separated by 5.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:16:02.74 +60:37:00.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:02.74 +60:37:00.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:02.74 +60:37:00.8: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 02 16 02.74 +60 37 00.8 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
target,2461170.9112,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260510.4112 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.76 01:43:03.23 +58:57:15.0
129.55608 -3.25214 galactic Cas Second-epoch detections are separated by 1.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.7767+58.9545 | 01:43:03.23 +58:57:15.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.236+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:03.23 +58:57:15.0: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:03.23 +58:57:15.0: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 43 03.23 +58 57 15.0 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.7767+58.9545,2461170.9112,10.76,0.05,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
ATO J025.7767+58.9545 20260510.4112 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.77 02:02:50.33 +60:13:59.9
131.68806 -1.41896 galactic Cas Second-epoch detections are separated by 2.0" and 2.3 pix
The object was found in VSX20" Gaia DR3 507950766893076736
Type: E
# Max. Min./Amp. JD0 Period
18.720 G 19.250 G 0.254094000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:50.33 +60:13:59.9: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:50.33 +60:13:59.9: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 02 02 50.33 +60 13 59.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507950766893076736,2461170.9112,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507950766893076736 20260510.4112 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 10.80 01:54:30.16 +59:06:35.1
130.96007 -2.77548 galactic Cas Second-epoch detections are separated by 1.6" and 2.9 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 J028.5927+59.1125 | 01:54:25.94 +59:06:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:30.16 +59:06:35.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:30.16 +59:06:35.1: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 54 30.16 +59 06 35.1 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J028.5927+59.1125,2461170.9112,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J028.5927+59.1125 20260510.4112 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 11.00 01:48:34.88 +58:41:32.6
130.31166 -3.35819 galactic Cas Second-epoch detections are separated by 3.9" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J027.1136+58.6801 | 01:48:31.31 +58:41:04.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:34.88 +58:41:32.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:34.88 +58:41:32.6: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 01 48 34.88 +58 41 32.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J027.1136+58.6801,2461170.9112,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J027.1136+58.6801 20260510.4112 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 11.12 02:09:18.24 +58:38:31.6
132.92997 -2.70994 galactic Per Second-epoch detections are separated by 1.1" and 3.0 pix
The object was found in VSX23" Gaia DR3 506787659695888768
Type: ROT
# Max. Min./Amp. JD0 Period
16.240 G 16.280 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:18.24 +58:38:31.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:18.24 +58:38:31.6: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 02 09 18.24 +58 38 31.6 11.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506787659695888768,2461170.9112,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506787659695888768 20260510.4112 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 11.24 02:04:34.65 +58:32:30.3
132.36857 -2.98355 galactic Per Second-epoch detections are separated by 3.0" and 2.1 pix
The object was found in VSX 1" Gaia DR3 506957087563281664
Type: ROT
# Max. Min./Amp. JD0 Period
13.840 G 13.870 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:04:34.65 +58:32:30.3: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:04:34.65 +58:32:30.3: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 02 04 34.65 +58 32 30.3 11.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506957087563281664,2461170.9112,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 506957087563281664 20260510.4112 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 10.4112 2461170.9112 9.47 02:18:22.27 +58:47:13.3
134.00333 -2.20342 galactic Per Second-epoch detections are separated by 1.8" and 2.8 pix
The object was found in VSX 6" NSVS J0218236+584716
Type: SR
# Max. Min./Amp. JD0 Period
12.694 r Y 0.560 r 2458351.79460 241.646383300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:22.27 +58:47:13.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:22.27 +58:47:13.3: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 10.4113* 02 18 22.27 +58 47 13.3 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0218236+584716,2461170.9112,9.47,0.05,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
NSVS J0218236+584716 20260510.4112 9.47CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461170.91150573 10.05.2026 09:52:24.095 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 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): 25045
Objects passed selection criteria: 24894
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 17085.8
Average stars matched: 15792.2 (92.4294 %)
Memory usage VmPeak: 128292 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 10 05:22:21 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461170.91150573 10.05.2026 09:52:24.095 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 124
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 130 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): 178985
Objects passed selection criteria: 178518
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 126776
Average stars matched: 117554 (92.7259 %)
Memory usage VmPeak: 2000200 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 10 05:30:16 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.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: 2461170.91098976
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:56.931 +61:59:37.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:56.931 +61:59:37.57
Angular distance between the image centers 0.0559 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:58.102 +61:59:24.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:58.102 +61:59:24.79
Angular distance between the image centers 0.0578 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:56.931 +61:59:37.57
Second-epoch second image center 01:42:58.102 +61:59:24.79
Angular distance between the image centers 0.00422 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.iUNieFi8oy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.J8U8uJqNxV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits &> /tmp/tmp.pwb3jy9v9q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits &> /tmp/tmp.OIMmgQFCrU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929150
a=0.000000 b=1.000000 c=22.929150
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.8)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.7 pix fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
2.6 pix fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
14.0 mag. fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
14.0 mag. fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.iUNieFi8oy (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 266 matched stars entering correct_measured_positions(), 9996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 337 matched stars entering correct_measured_positions(), 10041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.88"
Excluding outliers - 331 stars left (next iteration limit 292)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.J8U8uJqNxV (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.pwb3jy9v9q (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=958, passed=13349
Got 13349 stars (including 12386 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 13349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 13051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 13051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 13035 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 974 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OIMmgQFCrU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=989, passed=13527
Got 13527 stars (including 12532 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat
util/solve_plate_with_UCAC5 got 13527 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 13207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 13204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 13204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 970 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits'
Preparing the HTML report for the field Cas-03-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 08339_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 08339_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:20:32.65 +62:32:01.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06468_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 06468_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:54:23.50 +63:40:08.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17307_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 17307_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:25:50.48 +60:14:07.4 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:56.931 +61:59:37.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:56.931 +61:59:37.57
Angular distance between the image centers 0.0559 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:58.102 +61:59:24.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:58.102 +61:59:24.79
Angular distance between the image centers 0.0578 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:56.931 +61:59:37.57
Second-epoch second image center 01:42:58.102 +61:59:24.79
Angular distance between the image centers 0.00422 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.lFiwYZdW1V
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.YYhDOEFmDo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits &> /tmp/tmp.QaIgKu9SS0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits &> /tmp/tmp.v1WudSVEuF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.035150
a=0.000000 b=1.000000 c=20.035150
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.76
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=4.4)
Read 218998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9707 to 45.8168 deg, Dec +55.3262 to +67.4140 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9707 to 45.8168 deg, Dec 55.3262 to 67.4140 deg
Loaded 26295 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10859 out of 16691 total matches.
Matched with Tycho-2 16691 out of 218998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 104 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
12.8 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
12.7 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
11.4 mag. fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
11.4 mag. fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
All-image limiting magnitude estimate: 11.4 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.lFiwYZdW1V (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=35398, passed=222522
Got 222522 stars (including 186791 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 222522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 275 matched stars entering correct_measured_positions(), 212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 264 matched stars entering correct_measured_positions(), 49591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 434 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 49636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
Accuracy estimation diagnostic: 344 matched stars entering correct_measured_positions(), 64908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.78"
Excluding outliers - 344 stars left (next iteration limit 290)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.YYhDOEFmDo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=35098, passed=218974
Got 218974 stars (including 183551 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 218974 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QaIgKu9SS0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=8608, passed=90886
Got 90886 stars (including 82176 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 90886 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 89443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 89441 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 89387 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 971 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.v1WudSVEuF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=8741, passed=91597
Got 91597 stars (including 82750 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat
util/solve_plate_with_UCAC5 got 91597 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
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: 971 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 90408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
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: 969 matched stars entering correct_measured_positions(), 90407 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 90355 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 968 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-51-39_20.00sec_-5.00C_LIGHT_0086.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-10_CI_Cas-03-Q2b1x1_045405_TTUQ2b1x1_2838645_FPFapQOl/wcs_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087.fits
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:37.00 +63:57:53.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:46.59 +58:00:39.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:35.90 +64:25:06.5: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:01.35 +57:40:46.4: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:24.95 +64:28:44.6: 12.22 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:54.80 +58:10:52.1: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:05.11 +64:43:58.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:37.00 +63:57:53.6: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:35.90 +64:25:06.5: 13.69 +/- 0.04 detection
Forced photometry filter KEPT candidate at 01:26:37.00 +63:57:53.6: ref_mag=13.46 +/- 0.03 new_mean_mag=10.7605 delta=2.70 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:35.02 +57:33:10.4: 11.95 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter KEPT candidate at 02:01:35.90 +64:25:06.5: ref_mag=13.69 +/- 0.04 new_mean_mag=10.7496 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:54.80 +58:10:52.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Forced photometry filter KEPT candidate at 01:58:54.80 +58:10:52.1: ref_mag=13.23 +/- 0.03 new_mean_mag=10.8396 delta=2.39 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:46.59 +58:00:39.0: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Forced photometry filter KEPT candidate at 01:50:46.59 +58:00:39.0: ref_mag=13.62 +/- 0.04 new_mean_mag=10.7801 delta=2.84 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:24.95 +64:28:44.6: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:01.35 +57:40:46.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Forced photometry filter KEPT candidate at 01:14:01.35 +57:40:46.4: ref_mag=13.61 +/- 0.04 new_mean_mag=10.6324 delta=2.98 (need > 0.90)
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter KEPT candidate at 01:11:24.95 +64:28:44.6: ref_mag=13.59 +/- 0.04 new_mean_mag=10.6521 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:05.11 +64:43:58.6: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 01:07:05.11 +64:43:58.6: ref_mag=13.36 +/- 0.03 new_mean_mag=10.7833 delta=2.58 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:35.02 +57:33:10.4: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter KEPT candidate at 01:07:35.02 +57:33:10.4: ref_mag=13.41 +/- 0.03 new_mean_mag=10.6359 delta=2.78 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:36.50 +58:59:34.5: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:01.46 +59:16:32.1: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:36.50 +58:59:34.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 01:57:36.50 +58:59:34.5: ref_mag=13.33 +/- 0.03 new_mean_mag=10.3789 delta=2.95 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:01.46 +59:16:32.1: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Forced photometry filter KEPT candidate at 01:33:01.46 +59:16:32.1: ref_mag=13.85 +/- 0.05 new_mean_mag=10.6646 delta=3.19 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:43.71 +64:18:30.2: 11.67 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:43.71 +64:18:30.2: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Forced photometry filter KEPT candidate at 01:22:43.71 +64:18:30.2: ref_mag=13.14 +/- 0.03 new_mean_mag=10.2635 delta=2.87 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:17.51 +65:05:27.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:17.51 +65:05:27.9: 13.55 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:46.44 +57:24:46.4: 13.31 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter KEPT candidate at 01:06:17.51 +65:05:27.9: ref_mag=13.55 +/- 0.03 new_mean_mag=10.2332 delta=3.32 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:52.26 +63:48:34.5: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:26.15 +64:32:07.7: 12.71 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:46.44 +57:24:46.4: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter KEPT candidate at 01:13:46.44 +57:24:46.4: ref_mag=13.31 +/- 0.03 new_mean_mag=10.3872 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:52.26 +63:48:34.5: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 01:57:52.26 +63:48:34.5: ref_mag=13.27 +/- 0.02 new_mean_mag=10.3526 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:26.15 +64:32:07.7: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.07
Forced photometry filter KEPT candidate at 01:36:26.15 +64:32:07.7: ref_mag=13.93 +/- 0.07 new_mean_mag=10.3714 delta=3.56 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:16.86 +57:28:05.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:16.86 +57:28:05.4: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 01:15:16.86 +57:28:05.4: ref_mag=12.39 +/- 0.01 new_mean_mag=9.5828 delta=2.81 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:35.81 +57:57:40.7: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:53.15 +58:16:50.2: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:35.81 +57:57:40.7: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter KEPT candidate at 01:26:35.81 +57:57:40.7: ref_mag=13.29 +/- 0.03 new_mean_mag=10.5152 delta=2.77 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:53.15 +58:16:50.2: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.05
Forced photometry filter KEPT candidate at 01:54:53.15 +58:16:50.2: ref_mag=13.59 +/- 0.05 new_mean_mag=10.5519 delta=3.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:58.20 +60:30:25.1: 12.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:58.20 +60:30:25.1: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.06
Forced photometry filter KEPT candidate at 01:14:58.20 +60:30:25.1: ref_mag=13.66 +/- 0.06 new_mean_mag=10.6170 delta=3.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:52.81 +64:15:31.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:48.89 +59:06:41.1: 10.01 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:52.81 +64:15:31.8: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Forced photometry filter KEPT candidate at 01:55:52.81 +64:15:31.8: ref_mag=13.80 +/- 0.05 new_mean_mag=10.6073 delta=3.19 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:48.89 +59:06:41.1: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.02
Forced photometry filter REJECTED candidate at 02:09:48.89 +59:06:41.1: ref_mag=10.66 +/- 0.02 new_mean_mag=10.6717 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:02.74 +60:37:00.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:02.74 +60:37:00.8: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 02:16:02.74 +60:37:00.8: ref_mag=13.74 +/- 0.04 new_mean_mag=10.6948 delta=3.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:03.23 +58:57:15.0: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:03.23 +58:57:15.0: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter KEPT candidate at 01:43:03.23 +58:57:15.0: ref_mag=13.71 +/- 0.04 new_mean_mag=10.7554 delta=2.96 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:50.33 +60:13:59.9: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:50.33 +60:13:59.9: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Forced photometry filter KEPT candidate at 02:02:50.33 +60:13:59.9: ref_mag=13.62 +/- 0.05 new_mean_mag=10.7554 delta=2.86 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:30.16 +59:06:35.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:30.16 +59:06:35.1: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Forced photometry filter KEPT candidate at 01:54:30.16 +59:06:35.1: ref_mag=13.66 +/- 0.04 new_mean_mag=10.7768 delta=2.88 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:34.88 +58:41:32.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:34.88 +58:41:32.6: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.06
Forced photometry filter KEPT candidate at 01:48:34.88 +58:41:32.6: ref_mag=14.04 +/- 0.06 new_mean_mag=10.9919 delta=3.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:18.24 +58:38:31.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:18.24 +58:38:31.6: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.05
Forced photometry filter KEPT candidate at 02:09:18.24 +58:38:31.6: ref_mag=13.74 +/- 0.05 new_mean_mag=11.1103 delta=2.63 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:04:34.65 +58:32:30.3: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:04:34.65 +58:32:30.3: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.06
Forced photometry filter KEPT candidate at 02:04:34.65 +58:32:30.3: ref_mag=13.96 +/- 0.06 new_mean_mag=11.2464 delta=2.71 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:22.27 +58:47:13.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:22.27 +58:47:13.3: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 02:18:22.27 +58:47:13.3: ref_mag=13.39 +/- 0.03 new_mean_mag=9.4663 delta=3.92 (need > 0.90)
Adding exclusion_list_local.txt__out153703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out260761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266064.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 55s
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: 30s
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Considering the candidate 247635_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247635_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247636_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247636_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247639_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247639_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:47:52.48 +61:11:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247652_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247652_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247659_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247659_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247662_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247662_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247664_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247664_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247669_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247669_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:39:23.87 +58:23:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247672_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247672_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247675_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247675_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247676_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247676_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247678_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247678_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247681_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247681_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247686_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247686_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247687_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247687_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247691_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247691_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247694_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247694_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 247695_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247695_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:32:21.94 +60:27:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247701_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247701_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:25:15.85 +64:40:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247704_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247704_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:10:37.50 +57:22:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247709_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247709_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:19:24.08 +58:26:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247717_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247717_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:03:21.70 +57:48:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247719_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247719_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 247720_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247720_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:12:40.96 +61:20:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247723_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247723_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:07:07.99 +57:44:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247726_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247726_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:55:14.56 +59:32:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247727_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 247727_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:43:59.14 +61:55:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247730_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 247730_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 248513_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 248513_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 251137_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 251137_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:44:02.09 +61:53:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251462_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 251462_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:19:10.99 +58:20:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252042_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 252042_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 252076_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 252076_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:38:00.43 +57:56:46.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252700_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 252700_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 254065_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 254065_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 254088_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 254088_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:28:15.34 +58:44:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254562_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 254562_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:58:16.24 +59:38:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255646_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 255646_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:26:41.01 +60:46:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256422_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 256422_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:16:08.59 +58:49:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256556_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 256556_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:20:10.82 +58:12:11.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 257266_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 257266_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:44:17.62 +61:53:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257366_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 257366_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:00:51.67 +58:31:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258008_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 258008_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:15:59.01 +63:12:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258596_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 258596_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:02:55.04 +64:24:59.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 258942_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 258942_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 259120_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 259120_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:04:26.82 +65:05:53.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259218_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 259218_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:00:36.65 +58:30:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259648_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 259648_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:19:03.74 +63:57:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259980_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 259980_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:58:40.27 +59:16:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259999_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 259999_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:42:33.35 +63:53:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260019_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260019_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:16:36.21 +64:57:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260175_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260175_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:33:23.12 +57:44:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260279_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260279_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:10:23.90 +60:01:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260286_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260286_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:13:30.27 +58:34:25.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 260299_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260299_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:44:01.90 +61:52:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260374_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260374_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:29:34.01 +63:19:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260385_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260385_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:04:48.29 +57:53:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260490_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260490_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:35:50.38 +61:27:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260694_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260694_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:58:04.31 +57:58:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260761_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 260761_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 260880_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 260880_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:43:06.81 +58:57:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261093_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 261093_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:47:18.22 +63:38:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261174_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 261174_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 261202_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 261202_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:19:40.86 +62:51:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261547_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 261547_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:38:33.57 +60:47:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261881_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 261881_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:48:39.57 +59:09:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261944_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 261944_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 261996_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 261996_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:01:15.03 +59:23:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262070_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 262070_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:11:50.26 +59:02:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262074_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 262074_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:14:00.46 +61:42:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262258_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 262258_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:10:32.76 +59:59:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262422_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 262422_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:08:30.55 +58:24:17.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262474_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 262474_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:38:11.84 +61:01:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262570_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 262570_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 262617_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 262617_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
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Considering the candidate 262899_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 262899_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:18:04.11 +65:36:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262947_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 262947_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 263080_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 263080_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263316_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 263316_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:02:53.81 +60:15:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263340_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 263340_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:17:21.69 +59:22:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263370_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 263370_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:59:05.92 +59:55:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263466_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 263466_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:03:25.13 +57:50:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263567_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 263567_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:43:12.51 +64:00:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263972_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 263972_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263987_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 263987_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:44:56.35 +59:46:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264139_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 264139_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264822_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 264822_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264873_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 264873_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265427_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 265427_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:02:40.28 +59:57:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265993_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 265993_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266064_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 266064_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266191_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 266191_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183006_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 183006_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:20:05.31 +58:13:56.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53389_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 53389_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:11:26.51 +64:12:06.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167582_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 167582_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:33:55.94 +59:13:57.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61006_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 61006_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:54:23.51 +63:40:08.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153703_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 153703_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 72532_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:45:35.29 +63:07:10.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 70271_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:20:32.60 +62:32:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234396_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 234396_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:29:32.95 +63:18:24.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 76113_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 02:02:02.04 +62:41:32.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 39378_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:47:55.24 +64:32:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146540_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 146540_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:25:50.57 +60:14:07.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35226_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087
The candidate 35226_fd_Cas-03-Q2b1x1_2026-05-10_04-52-24_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 01:11:42.14 +65:01:04.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 87s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:18:22.27 +58:47:13.3
01:26:37.00 +63:57:53.6
01:07:05.11 +64:43:58.6
01:50:46.59 +58:00:39.0
01:58:54.80 +58:10:52.1
02:01:35.90 +64:25:06.5
01:14:01.35 +57:40:46.4
01:07:35.02 +57:33:10.4
01:11:24.95 +64:28:44.6
01:57:36.50 +58:59:34.5
01:33:01.46 +59:16:32.1
01:22:43.71 +64:18:30.2
01:06:17.51 +65:05:27.9
01:13:46.44 +57:24:46.4
01:57:52.26 +63:48:34.5
01:36:26.15 +64:32:07.7
01:15:16.86 +57:28:05.4
01:26:35.81 +57:57:40.7
01:54:53.15 +58:16:50.2
01:14:58.20 +60:30:25.1
01:55:52.81 +64:15:31.8
02:16:02.74 +60:37:00.8
01:43:03.23 +58:57:15.0
02:02:50.33 +60:13:59.9
01:54:30.16 +59:06:35.1
01:48:34.88 +58:41:32.6
02:09:18.24 +58:38:31.6
02:04:34.65 +58:32:30.3
########### Completed Cas-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:26:37.00 +63:57:53.6
01:07:05.11 +64:43:58.6
01:50:46.59 +58:00:39.0
01:58:54.80 +58:10:52.1
02:01:35.90 +64:25:06.5
01:14:01.35 +57:40:46.4
01:07:35.02 +57:33:10.4
01:11:24.95 +64:28:44.6
01:57:36.50 +58:59:34.5
01:33:01.46 +59:16:32.1
01:22:43.71 +64:18:30.2
01:06:17.51 +65:05:27.9
01:13:46.44 +57:24:46.4
01:57:52.26 +63:48:34.5
01:36:26.15 +64:32:07.7
01:15:16.86 +57:28:05.4
01:26:35.81 +57:57:40.7
01:54:53.15 +58:16:50.2
01:14:58.20 +60:30:25.1
01:55:52.81 +64:15:31.8
02:16:02.74 +60:37:00.8
01:43:03.23 +58:57:15.0
02:02:50.33 +60:13:59.9
01:54:30.16 +59:06:35.1
01:48:34.88 +58:41:32.6
02:09:18.24 +58:38:31.6
02:04:34.65 +58:32:30.3
02:18:22.27 +58:47:13.3
###################################################################################
01:26:37.00 +63:57:53.6 -- not an asteroid (will add it to exclusion list)
01:07:05.11 +64:43:58.6 -- not an asteroid (will add it to exclusion list)
01:50:46.59 +58:00:39.0 -- not an asteroid (will add it to exclusion list)
01:58:54.80 +58:10:52.1 -- not an asteroid (will add it to exclusion list)
02:01:35.90 +64:25:06.5 -- not an asteroid (will add it to exclusion list)
01:14:01.35 +57:40:46.4 -- not an asteroid (will add it to exclusion list)
01:07:35.02 +57:33:10.4 -- not an asteroid (will add it to exclusion list)
01:11:24.95 +64:28:44.6 -- not an asteroid (will add it to exclusion list)
01:57:36.50 +58:59:34.5 -- not an asteroid (will add it to exclusion list)
01:33:01.46 +59:16:32.1 -- not an asteroid (will add it to exclusion list)
01:22:43.71 +64:18:30.2 -- not an asteroid (will add it to exclusion list)
01:06:17.51 +65:05:27.9 -- not an asteroid (will add it to exclusion list)
01:13:46.44 +57:24:46.4 -- not an asteroid (will add it to exclusion list)
01:57:52.26 +63:48:34.5 -- not an asteroid (will add it to exclusion list)
01:36:26.15 +64:32:07.7 -- not an asteroid (will add it to exclusion list)
01:15:16.86 +57:28:05.4 -- not an asteroid (will add it to exclusion list)
01:26:35.81 +57:57:40.7 -- not an asteroid (will add it to exclusion list)
01:54:53.15 +58:16:50.2 -- not an asteroid (will add it to exclusion list)
01:14:58.20 +60:30:25.1 -- not an asteroid (will add it to exclusion list)
01:55:52.81 +64:15:31.8 -- not an asteroid (will add it to exclusion list)
02:16:02.74 +60:37:00.8 -- not an asteroid (will add it to exclusion list)
01:43:03.23 +58:57:15.0 -- not an asteroid (will add it to exclusion list)
02:02:50.33 +60:13:59.9 -- not an asteroid (will add it to exclusion list)
01:54:30.16 +59:06:35.1 -- not an asteroid (will add it to exclusion list)
01:48:34.88 +58:41:32.6 -- not an asteroid (will add it to exclusion list)
02:09:18.24 +58:38:31.6 -- not an asteroid (will add it to exclusion list)
02:04:34.65 +58:32:30.3 -- not an asteroid (will add it to exclusion list)
02:18:22.27 +58:47:13.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:06:17.51 +65:05:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:05.11 +64:43:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:35.02 +57:33:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:24.95 +64:28:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:46.44 +57:24:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:01.35 +57:40:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:58.20 +60:30:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:16.86 +57:28:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:43.71 +64:18:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:35.81 +57:57:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:37.00 +63:57:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:01.46 +59:16:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:26.15 +64:32:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:03.23 +58:57:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:34.88 +58:41:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:46.59 +58:00:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:30.16 +59:06:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:53.15 +58:16:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:52.81 +64:15:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:36.50 +58:59:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:52.26 +63:48:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:54.80 +58:10:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:35.90 +64:25:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:50.33 +60:13:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:34.65 +58:32:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:18.24 +58:38:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:02.74 +60:37:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:22.27 +58:47:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:06:17.51 +65:05:27.9 -- not a known variable star
01:07:05.11 +64:43:58.6 -- not a known variable star
01:07:35.02 +57:33:10.4 -- not a known variable star
01:11:24.95 +64:28:44.6 -- not a known variable star
01:13:46.44 +57:24:46.4 -- not a known variable star
01:14:01.35 +57:40:46.4 -- not a known variable star
01:14:58.20 +60:30:25.1 -- a known variable star
01:15:16.86 +57:28:05.4 -- not a known variable star
01:22:43.71 +64:18:30.2 -- not a known variable star
01:26:35.81 +57:57:40.7 -- not a known variable star
01:26:37.00 +63:57:53.6 -- not a known variable star
01:33:01.46 +59:16:32.1 -- not a known variable star
01:36:26.15 +64:32:07.7 -- a known variable star
01:43:03.23 +58:57:15.0 -- not a known variable star
01:48:34.88 +58:41:32.6 -- not a known variable star
01:50:46.59 +58:00:39.0 -- not a known variable star
01:54:30.16 +59:06:35.1 -- not a known variable star
01:54:53.15 +58:16:50.2 -- not a known variable star
01:55:52.81 +64:15:31.8 -- not a known variable star
01:57:36.50 +58:59:34.5 -- not a known variable star
01:57:52.26 +63:48:34.5 -- a known variable star
01:58:54.80 +58:10:52.1 -- not a known variable star
02:01:35.90 +64:25:06.5 -- not a known variable star
02:02:50.33 +60:13:59.9 -- a known variable star
02:04:34.65 +58:32:30.3 -- a known variable star
02:09:18.24 +58:38:31.6 -- a known variable star
02:16:02.74 +60:37:00.8 -- not a known variable star
02:18:22.27 +58:47:13.3 -- a known variable star
Found 21 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
28 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 ####
01:06:17.51 +65:05:27.9
01:07:05.11 +64:43:58.6
01:07:35.02 +57:33:10.4
01:11:24.95 +64:28:44.6
01:13:46.44 +57:24:46.4
01:14:01.35 +57:40:46.4
01:14:58.20 +60:30:25.1
01:15:16.86 +57:28:05.4
01:22:43.71 +64:18:30.2
01:26:35.81 +57:57:40.7
01:26:37.00 +63:57:53.6
01:33:01.46 +59:16:32.1
01:36:26.15 +64:32:07.7
01:43:03.23 +58:57:15.0
01:48:34.88 +58:41:32.6
01:50:46.59 +58:00:39.0
01:54:30.16 +59:06:35.1
01:54:53.15 +58:16:50.2
01:55:52.81 +64:15:31.8
01:57:36.50 +58:59:34.5
01:57:52.26 +63:48:34.5
01:58:54.80 +58:10:52.1
02:01:35.90 +64:25:06.5
02:02:50.33 +60:13:59.9
02:04:34.65 +58:32:30.3
02:09:18.24 +58:38:31.6
02:16:02.74 +60:37:00.8
02:18:22.27 +58:47:13.3
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461170.91098976 -observatory V36
02:48:31.15 +15:36:20.9 Mercury (-1.7mag)
05:12:53.55 +24:17:15.6 Venus (-3.9mag)
01:27:01.98 +08:14:53.9 Mars (1.2mag)
07:26:33.14 +22:20:48.9 Jupiter (-2.0mag)
00:39:29.77 +01:51:56.4 Saturn (0.9mag)
03:53:14.76 +20:04:49.5 Uranus (5.8mag)
00:13:45.01 +00:02:41.4 Neptune (7.8mag)
20:34:14.31 -22:55:51.6 Pluto (14.5mag)
21:55:02.76 -14:26:07.4 Moon (-10.2mag)
-rw-r--r-- 1 apache apache 363 May 10 05:22 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461170.91098976:
07:26:26.58 +22:21:04.8 Io (5.9mag)
07:26:27.12 +22:21:06.0 Europa (6.0mag)
07:26:15.63 +22:21:30.7 Ganymede (5.5mag)
07:26:03.58 +22:21:56.6 Callisto (6.7mag)
07:28:35.73 +21:59:41.1 Himalia (15.5mag)
07:26:31.95 +22:20:50.9 Thebe (16.4mag)
07:29:03.97 +22:26:53.2 Elara (17.4mag)
07:27:03.25 +22:47:59.8 Pasiphae (17.6mag)
07:34:13.40 +22:20:41.3 Carme (18.7mag)
00:39:33.08 +01:51:39.9 Titan (8.7mag)
00:39:35.44 +01:51:59.0 Rhea (10.0mag)
00:39:15.79 +01:49:56.1 Iapetus (11.4mag)
00:39:26.30 +01:52:26.0 Hyperion (14.7mag)
00:40:44.44 +01:57:50.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 10 05:22 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461170.91098976:
16:55:24.16 -28:55:56.2 JWST
16:07:26.59 +50:14:35.5 Chandra
09:16:07.96 -52:54:35.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 10 05:22 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461170.91098976 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
07:34:58.88 +26:20:19.3 17.7mag P/2009 WX51 (Catalina)
18:55:36.70 -30:25:42.7 13.7mag P/2010 H2 (Vales)
05:26:25.43 -68:41:07.0 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:39:03.36 +31:38:24.6 17.4mag C/2017 K2 (PANSTARRS)
17:25:20.06 +13:12:22.9 17.7mag C/2021 G2 (ATLAS)
23:14:30.77 +30:18:50.3 17.1mag C/2022 E2 (ATLAS)
04:58:33.88 +26:36:38.1 16.2mag C/2022 N2 (PANSTARRS)
09:12:08.84 +31:51:20.4 16.4mag C/2022 QE78 (ATLAS)
08:37:28.38 +02:06:28.0 17.5mag C/2022 R6 (PANSTARRS)
18:44:52.34 +20:22:04.6 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:31:11.00 -11:10:50.7 17.5mag P/2023 B1 (PANSTARRS)
09:00:30.82 -08:24:58.4 17.9mag C/2023 F3 (ATLAS)
22:12:09.64 +64:31:44.2 17.6mag C/2023 H5 (Lemmon)
18:48:08.21 -04:31:00.4 13.9mag C/2023 R1 (PANSTARRS)
16:30:29.71 +88:13:36.7 17.9mag C/2023 X2 (Lemmon)
06:36:01.38 +63:37:27.2 17.4mag C/2024 A1 (ATLAS)
06:00:18.79 +24:12:10.2 12.4mag C/2024 E1 (Wierzchos)
16:01:03.02 +10:10:42.0 17.3mag C/2024 G6 (ATLAS)
20:23:24.76 +22:19:52.9 14.3mag C/2024 J3 (ATLAS)
03:49:22.25 -19:00:34.3 16.2mag C/2024 T5 (ATLAS)
05:38:45.48 +39:50:53.3 17.8mag C/2025 J1 (Borisov)
12:14:17.31 +53:04:17.9 16.3mag C/2025 L1 (ATLAS)
05:30:15.91 -07:23:36.5 10.2mag C/2025 R3 (PANSTARRS)
12:44:44.95 +04:12:57.5 17.3mag C/2025 Y1 (ATLAS)
05:23:26.15 +01:24:23.9 17.7mag C/2026 A1 (MAPS)
01:02:18.03 +40:47:20.2 15.3mag C/2026 B2 (Sun-Gao)
19:29:57.75 -08:27:55.0 10.4mag 10P/Tempel
14:29:58.49 -00:03:02.7 16.2mag 24P/Schaumasse
10:59:04.33 -00:57:28.9 15.8mag 29P/Schwassmann-Wachmann
10:42:37.25 -02:46:16.2 17.4mag 43P/Wolf-Harrington
02:26:45.20 +21:28:18.3 17.4mag 47P/Ashbrook-Jackson
07:59:04.33 +31:24:42.7 16.9mag 63P/Wild
23:58:16.88 -08:45:24.5 15.7mag 65P/Gunn
05:12:47.95 +28:26:53.1 16.2mag 76P/West-Kohoutek-Ikemura
02:00:54.07 +12:47:57.6 14.1mag 78P/Gehrels
00:11:47.03 -02:19:20.4 15.0mag 88P/Howell
03:22:59.04 +26:20:41.9 15.1mag 93P/Lovas
05:44:35.93 +33:13:14.3 15.9mag 123P/West-Hartley
09:02:25.75 +27:14:48.8 16.3mag 124P/Mrkos
03:11:53.45 +16:54:08.5 16.4mag 128P/Shoemaker-Holt
03:35:58.89 +17:06:04.4 17.6mag 131P/Mueller
03:37:53.08 +19:01:06.0 11.3mag 141P/Machholz
03:42:20.91 +13:03:58.9 11.3mag 141P-A/Machholz
02:22:31.21 +09:12:04.9 10.6mag 141P-D/Machholz
02:36:14.86 -29:24:42.6 17.8mag 161P/Hartley-IRAS
02:12:07.69 +10:44:38.5 14.9mag 162P/SidingSpring
17:12:46.63 -10:57:56.0 16.1mag 235P/LINEAR
06:28:57.97 +35:50:27.9 17.1mag 240P/NEAT
07:53:39.59 -02:58:33.3 17.9mag 242P/Spahr
23:18:17.74 -13:32:45.1 17.2mag 260P/McNaught
02:51:31.56 +26:24:44.7 17.8mag 295P/LINEAR
15:30:33.66 +08:10:51.5 17.4mag 391P/Kowalski
07:46:35.92 +21:16:18.6 17.8mag 450P/LONEOS
06:13:20.54 +43:35:16.2 17.7mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K May 10 05:22 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
21:35:33.81 -14:05:16.30 2026-05-6.29 14.51
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:35:33.81 -14:05:16.30 2026-05-6.29 14.51
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
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
-rw-r--r-- 1 apache apache 188K May 10 05:22 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:47:41.180 +44:21:12.63 AT 2026ldg 2026-03-10.69 22.07
14:06:50.300 +03:38:25.84 AT 2026ldf 2026-03-29.82 21.68
13:46:12.200 +04:59:50.61 AT 2026lde 2026-04-22.73 22.17
18:24:40.506 +25:34:34.40 AT 2026ldd 2026-04-30.29 19.2562
18:29:31.904 -10:55:31.47 AT 2026ldc 2026-04-29.51 17.844
19:01:56.370 +18:27:54.50 AT 2026ldb 2026-04-30.25 17.1
22:14:40.686 +05:04:50.71 SN 2026lda 2026-04-29.49 19.207
19:21:44.270 +17:53:08.50 AT 2026lcz 2026-04-30.29 15.4
09:54:38.926 +01:39:54.85 AT 2026lcy 2026-04-21.03 23.1907
09:57:55.638 +02:13:40.62 AT 2026lcx 2026-04-21.04 23.5642
20:42:38.405 +07:13:35.97 AT 2026lcw 2026-04-28.45 16.998
10:02:36.427 +03:01:31.29 AT 2026lcv 2026-04-21.03 23.1103
18:26:46.110 +15:07:42.10 AT 2026lcu 2026-04-27.86 18.24
10:04:58.540 +02:53:02.41 AT 2026lct 2026-04-30.07 22.2176
19:15:02.800 +19:30:54.00 AT 2026lcs 2026-04-30.29 16.4
10:04:58.691 +01:52:31.48 AT 2026lcr 2026-04-21.04 23.3217
19:14:18.020 +20:21:21.90 AT 2026lcq 2026-04-30.29 17.5
18:21:27.688 +27:26:09.36 AT 2026lcp 2026-03-12.49 20.0198
11:32:42.159 +17:32:08.36 AT 2026lco 2026-04-29.26 19.641
10:31:32.860 +08:00:34.70 AT 2026lcn 2026-04-07.21 20.5201
-rw-r--r-- 1 apache apache 30K May 10 05:22 tns_transients_list.txt
