This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL
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 14.3988 2461174.8988 11.71 01:58:29.33 +63:45:09.2
130.26367 1.83936 galactic Cas Second-epoch detections are separated by 1.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:58:29.33 +63:45:09.2 (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 01:58:29.33 +63:45:09.2: 13.00 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:29.33 +63:45:09.2: 14.47 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 58 29.33 +63 45 09.2 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.70 01:55:28.41 +63:18:58.4
130.04799 1.33264 galactic Cas Second-epoch detections are separated by 2.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:55:28.41 +63:18:58.4 (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 01:55:28.41 +63:18:58.4: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:28.41 +63:18:58.4: 14.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.38 +/- 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 14.3988* 01 55 28.41 +63 18 58.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.71 01:26:31.82 +61:19:28.1
127.13002 -1.26091 galactic Cas Second-epoch detections are separated by 1.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:26:31.82 +61:19:28.1 (user input) | T | P | (position from user input) J-Ks=1.481+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:31.82 +61:19:28.1: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:31.82 +61:19:28.1: 14.62 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.09
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 14.3988* 01 26 31.82 +61 19 28.1 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.47 01:28:22.63 +57:57:58.8
127.83045 -4.55365 galactic Cas Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J022.1117+57.9737 | 01:28:22.63 +57:57:58.8 (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 01:28:22.63 +57:57:58.8: 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 01:28:22.63 +57:57:58.8: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 14.3988* 01 28 22.63 +57 57 58.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.1117+57.9737,2461174.8988,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.1117+57.9737 20260514.3988 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.40 01:41:51.95 +60:08:24.8
129.17475 -2.11887 galactic Cas Second-epoch detections are separated by 1.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.4532+60.1341 | 01:41:51.95 +60:08:24.8 (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 01:41:51.95 +60:08:24.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:51.95 +60:08:24.8: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 41 51.95 +60 08 24.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.4532+60.1341,2461174.8988,11.40,0.05,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
ATO J025.4532+60.1341 20260514.3988 11.40CV 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 14.3988 2461174.8988 11.31 01:37:23.78 +59:20:13.2
128.77043 -3.01277 galactic Cas Second-epoch detections are separated by 2.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:37:23.78 +59:20:13.2 (user input) | T | P | (position from user input) J-Ks=0.300+/-0.042 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:23.78 +59:20:13.2: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:23.78 +59:20:13.2: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 37 23.78 +59 20 13.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.43 01:11:19.87 +61:17:56.6
125.31878 -1.48047 galactic Cas Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:11:19.87 +61:17:56.6 (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 01:11:19.87 +61:17:56.6: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:19.87 +61:17:56.6: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 14.3988* 01 11 19.87 +61 17 56.6 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.43,0.05,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 20260514.3988 11.43CV 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 14.3988 2461174.8988 11.39 01:33:12.70 +61:16:56.9
127.92956 -1.18327 galactic Cas Second-epoch detections are separated by 0.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:12.70 +61:16:56.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:12.70 +61:16:56.9: 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 01:33:12.70 +61:16:56.9: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 14.3988* 01 33 12.70 +61 16 56.9 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.22 01:19:46.43 +63:03:13.4
126.13562 0.35837 galactic Cas Second-epoch detections are separated by 3.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:19:46.43 +63:03:13.4 (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 01:19:46.43 +63:03:13.4: 12.57 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:46.43 +63:03:13.4: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 19 46.43 +63 03 13.4 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.20 01:54:24.55 +61:25:41.9
130.38801 -0.52850 galactic Cas Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 508314812625727104 | 01:54:25.02 +61:25:14.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.896+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:24.55 +61:25:41.9: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:24.55 +61:25:41.9: 14.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 14.3988* 01 54 24.55 +61 25 41.9 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508314812625727104,2461174.8988,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508314812625727104 20260514.3988 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.42 01:16:38.51 +63:11:33.2
125.76914 0.45973 galactic Cas Second-epoch detections are separated by 4.0" and 6.5 pix
The object was found in VSX 3" Gaia DR3 523149870180930816
Type: ROT
# Max. Min./Amp. JD0 Period
13.980 G 14.010 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:38.51 +63:11:33.2: 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 01:16:38.51 +63:11:33.2: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 14.3988* 01 16 38.51 +63 11 33.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523149870180930816,2461174.8988,11.42,0.05,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 523149870180930816 20260514.3988 11.42CV 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 14.3988 2461174.8988 11.23 01:12:41.30 +61:18:09.6
125.48096 -1.46386 galactic Cas Second-epoch detections are separated by 0.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:41.30 +61:18:09.6 (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 01:12:41.30 +61:18:09.6: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:41.30 +61:18:09.6: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 14.3988* 01 12 41.30 +61 18 09.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.08 01:05:42.77 +62:52:34.3
124.55812 0.04953 galactic Cas Second-epoch detections are separated by 3.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:05:42.77 +62:52:34.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:42.77 +62:52:34.3: 11.05 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:42.77 +62:52:34.3: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 14.3988* 01 05 42.77 +62 52 34.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.15 01:08:39.10 +60:32:42.8
125.04821 -2.25577 galactic Cas Second-epoch detections are separated by 1.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:39.10 +60:32:42.8 (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 01:08:39.10 +60:32:42.8: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:39.10 +60:32:42.8: 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 14.3988* 01 08 39.10 +60 32 42.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.31 01:13:01.38 +61:01:00.6
125.54495 -1.74536 galactic Cas Second-epoch detections are separated by 2.3" and 6.3 pix
The object was found in VSX 6" Gaia DR3 522455906553654144
Type:
# Max. Min./Amp. JD0 Period
16.000 G 16.860 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:01.38 +61:01:00.6: 12.29 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:01.38 +61:01:00.6: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 14.3988* 01 13 01.38 +61 01 00.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522455906553654144,2461174.8988,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522455906553654144 20260514.3988 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.23 01:38:38.44 +61:15:26.1
128.57673 -1.09610 galactic Cas Second-epoch detections are separated by 1.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:38:38.44 +61:15:26.1 (user input) | T | P | (position from user input) J-Ks=0.177+/-0.051 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:38.44 +61:15:26.1: 11.60 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:38.44 +61:15:26.1: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 14.3988* 01 38 38.44 +61 15 26.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.12 01:12:09.70 +58:47:54.8
125.61965 -3.96500 galactic Cas Second-epoch detections are separated by 1.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:09.70 +58:47:54.8 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:09.70 +58:47:54.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:09.70 +58:47:54.8: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 14.3988* 01 12 09.70 +58 47 54.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.12,0.05,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
target 20260514.3988 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 14.3988 2461174.8988 11.12 01:07:36.78 +58:09:26.4
125.07112 -4.64722 galactic Cas Second-epoch detections are separated by 0.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:36.78 +58:09:26.4 (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 01:07:36.78 +58:09:26.4: 12.66 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:36.78 +58:09:26.4: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 07 36.78 +58 09 26.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.12,0.05,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
target 20260514.3988 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 14.3988 2461174.8988 11.02 01:25:27.50 +59:27:17.3
127.24903 -3.13148 galactic Cas Second-epoch detections are separated by 0.3" and 5.9 pix
The object was found in VSX 5" Gaia DR3 510073344036983552
Type: ROT
# Max. Min./Amp. JD0 Period
14.460 G 14.520 G 1.820050000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:27.50 +59:27:17.3: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:27.50 +59:27:17.3: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 25 27.50 +59 27 17.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510073344036983552,2461174.8988,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510073344036983552 20260514.3988 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.94 01:47:51.38 +61:11:14.0
129.67765 -0.94343 galactic Cas Second-epoch detections are separated by 2.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511214048684134528 | 01:47:54.00 +61:10:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.225+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:51.38 +61:11:14.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:51.38 +61:11:14.0: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 14.3988* 01 47 51.38 +61 11 14.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511214048684134528,2461174.8988,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511214048684134528 20260514.3988 10.94CV 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 14.3988 2461174.8988 11.24 01:35:41.55 +61:13:14.2
128.23406 -1.19473 galactic Cas Second-epoch detections are separated by 1.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:35:41.55 +61:13:14.2 (user input) | T | P | (position from user input) J-Ks=2.864+/- (Very red!)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:41.55 +61:13:14.2: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:41.55 +61:13:14.2: 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 14.3988* 01 35 41.55 +61 13 14.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.24,0.05,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
target 20260514.3988 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 14.3988 2461174.8988 11.03 01:10:03.10 +57:48:14.8
125.41877 -4.97773 galactic Cas Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:10:03.10 +57:48:14.8 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:03.10 +57:48:14.8: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:03.10 +57:48:14.8: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 14.3988* 01 10 03.10 +57 48 14.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.08 01:10:11.76 +59:17:25.9
125.32927 -3.49388 galactic Cas Second-epoch detections are separated by 1.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.5672+59.2942 | 01:10:11.76 +59:17:25.9 (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 01:10:11.76 +59:17:25.9: 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 01:10:11.76 +59:17:25.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 10 11.76 +59 17 25.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.5672+59.2942,2461174.8988,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.5672+59.2942 20260514.3988 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.08 01:20:42.36 +66:02:08.4
125.90214 3.33285 galactic Cas Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:20:42.36 +66:02:08.4 (user input) | T | P | (position from user input) J-Ks=1.055+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:42.36 +66:02:08.4: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:42.36 +66:02:08.4: 13.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 14.3988* 01 20 42.36 +66 02 08.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.07 01:51:47.25 +58:37:59.8
130.73180 -3.32155 galactic Cas Second-epoch detections are separated by 2.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506225156418009984 | 01:51:45.68 +58:37:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.890+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:47.25 +58:37:59.8: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:47.25 +58:37:59.8: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 14.3988* 01 51 47.25 +58 37 59.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506225156418009984,2461174.8988,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506225156418009984 20260514.3988 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.11 01:15:44.74 +60:02:47.1
125.96517 -2.68209 galactic Cas Second-epoch detections are separated by 0.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:15:44.74 +60:02:47.1 (user input) | T | P | (position from user input) J-Ks=0.321+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:44.74 +60:02:47.1: 12.40 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:44.74 +60:02:47.1: 13.82 +/- 0.05 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 14.3988* 01 15 44.74 +60 02 47.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.98 01:29:02.54 +58:46:11.6
127.80057 -3.74593 galactic Cas Second-epoch detections are separated by 2.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J012906.85+584639.3 | 01:29:06.84 +58:46:39.2 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:02.54 +58:46:11.6: 12.74 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:02.54 +58:46:11.6: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 14.3988* 01 29 02.54 +58 46 11.6 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
ASASSN-V J012906.85+584639.3,2461174.8988,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J012906.85+584639.3 20260514.3988 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.89 01:05:20.99 +64:15:24.0
124.44226 1.42572 galactic Cas Second-epoch detections are separated by 3.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:05:20.99 +64:15:24.0 (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 01:05:20.99 +64:15:24.0: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:20.99 +64:15:24.0: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 14.3988* 01 05 20.99 +64 15 24.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.97 01:07:39.23 +59:59:20.2
124.96077 -2.81891 galactic Cas Second-epoch detections are separated by 0.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:39.23 +59:59:20.2 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.23 +59:59:20.2: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.23 +59:59:20.2: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 14.3988* 01 07 39.23 +59 59 20.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.97 01:24:54.95 +59:41:48.8
127.14915 -2.90045 galactic Cas Second-epoch detections are separated by 2.7" and 5.5 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 | 01:24:54.95 +59:41:48.8 (user input) | T | P | (position from user input) J-Ks=0.217+/-0.043 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:54.95 +59:41:48.8: 13.01 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:54.95 +59:41:48.8: 13.99 +/- 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 14.3988* 01 24 54.95 +59 41 48.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.80 02:06:09.31 +62:45:45.0
131.36242 1.12014 galactic Cas Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:06:09.31 +62:45:45.0 (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 02:06:09.31 +62:45:45.0: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:06:09.31 +62:45:45.0: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 02 06 09.31 +62 45 45.0 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
target,2461174.8988,10.80,0.05,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
target 20260514.3988 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 14.3988 2461174.8988 10.86 01:09:21.52 +64:35:19.4
124.85376 1.78387 galactic Cas Second-epoch detections are separated by 4.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:09:21.52 +64:35:19.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:21.52 +64:35:19.4: 12.72 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:21.52 +64:35:19.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 09 21.52 +64 35 19.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.66 01:26:36.61 +59:41:36.1
127.36173 -2.87553 galactic Cas Second-epoch detections are separated by 1.9" and 5.8 pix
The object was found in VSX 2" Gaia DR3 510083239641443712
Type: ROT
# Max. Min./Amp. JD0 Period
13.540 G 13.590 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:36.61 +59:41:36.1: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:36.61 +59:41:36.1: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 14.3988* 01 26 36.61 +59 41 36.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510083239641443712,2461174.8988,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510083239641443712 20260514.3988 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.85 01:11:44.58 +61:13:58.7
125.37330 -1.54249 galactic Cas Second-epoch detections are separated by 2.2" and 6.1 pix
The object was found in VSX 2" ZTF J011144.73+611356.9
Type: RS
# Max. Min./Amp. JD0 Period
13.552 r Y 0.107 r 2458423.79830 1.359407700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:44.58 +61:13:58.7: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:44.58 +61:13:58.7: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 11 44.58 +61 13 58.7 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
ZTF J011144.73+611356.9,2461174.8988,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011144.73+611356.9 20260514.3988 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.61 01:07:31.53 +61:28:29.3
124.85186 -1.33696 galactic Cas Second-epoch detections are separated by 1.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:31.53 +61:28:29.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:31.53 +61:28:29.3: 12.60 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:31.53 +61:28:29.3: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 07 31.53 +61 28 29.3 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,2461174.8988,10.61,0.05,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 20260514.3988 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 14.3988 2461174.8988 10.53 01:08:23.16 +61:35:11.1
124.94706 -1.21900 galactic Cas Second-epoch detections are separated by 0.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 522537991967390976 | 01:08:20.09 +61:35:51.7 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A0 1935BSD...C01....0S BSD 8-1620
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:23.16 +61:35:11.1: 12.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:23.16 +61:35:11.1: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 14.3988* 01 08 23.16 +61 35 11.1 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522537991967390976,2461174.8988,10.53,0.05,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 522537991967390976 20260514.3988 10.53CV 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 14.3988 2461174.8988 10.44 01:38:10.70 +60:44:57.0
128.61369 -1.60592 galactic Cas Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:38:10.70 +60:44:57.0 (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 01:38:10.70 +60:44:57.0: 11.84 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:10.70 +60:44:57.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 14.3988* 01 38 10.70 +60 44 57.0 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,2461174.8988,10.44,0.05,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 20260514.3988 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 14.3988 2461174.8988 9.60 01:20:24.32 +59:10:25.8
126.64249 -3.48906 galactic Cas Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J020.1204+59.1623 | 01:20:25.01 +59:10:05.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.296+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:24.32 +59:10:25.8: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:24.32 +59:10:25.8: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 14.3988* 01 20 24.32 +59 10 25.8 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
ATO J020.1204+59.1623,2461174.8988,9.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J020.1204+59.1623 20260514.3988 9.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.46 01:29:33.67 +63:19:32.1
127.19510 0.76983 galactic Cas Second-epoch detections are separated by 4.8" and 5.2 pix
The object was found in VSX14" Gaia DR3 512422828587465216
Type: S
# Max. Min./Amp. JD0 Period
14.920 G 15.600 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:33.67 +63:19:32.1: 12.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:33.67 +63:19:32.1: 13.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 14.3988* 01 29 33.67 +63 19 32.1 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512422828587465216,2461174.8988,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512422828587465216 20260514.3988 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.90 01:18:48.42 +64:12:23.7
125.90445 1.49291 galactic Cas Second-epoch detections are separated by 1.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:48.42 +64:12:23.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:48.42 +64:12:23.7: 11.73 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:48.42 +64:12:23.7: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 14.3988* 01 18 48.42 +64 12 23.7 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.89 01:11:56.58 +58:41:06.3
125.60043 -4.08038 galactic Cas Second-epoch detections are separated by 1.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.9933+58.6776 | 01:11:56.58 +58:41:06.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:56.58 +58:41:06.3: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:56.58 +58:41:06.3: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 14.3988* 01 11 56.58 +58 41 06.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.9933+58.6776,2461174.8988,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.9933+58.6776 20260514.3988 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.02 01:31:48.39 +64:22:29.0
127.28049 1.84435 galactic Cas Second-epoch detections are separated by 1.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.39 +64:22:29.0 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.39 +64:22:29.0: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.39 +64:22:29.0: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 14.3988* 01 31 48.39 +64 22 29.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.91 01:38:34.53 +57:58:02.8
129.16849 -4.33239 galactic Cas Second-epoch detections are separated by 2.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.6398+57.9682 | 01:38:34.52 +57:58:32.1 (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 01:38:34.53 +57:58:02.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:34.53 +57:58:02.8: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 14.3988* 01 38 34.53 +57 58 02.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.6398+57.9682,2461174.8988,10.91,0.05,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 J024.6398+57.9682 20260514.3988 10.91CV 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 14.3988 2461174.8988 11.14 01:13:38.83 +58:10:53.0
125.86527 -4.56381 galactic Cas Second-epoch detections are separated by 2.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J018.4234+58.1762 | 01:13:41.63 +58:10:34.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.593+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:38.83 +58:10:53.0: 13.07 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:38.83 +58:10:53.0: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 13 38.83 +58 10 53.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.4234+58.1762,2461174.8988,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.4234+58.1762 20260514.3988 11.14CV 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 14.3988 2461174.8988 11.04 01:26:05.42 +59:01:17.1
127.38703 -3.55026 galactic Cas Second-epoch detections are separated by 1.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.5231+59.0209 | 01:26:05.42 +59:01:17.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.42 +59:01:17.1: 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 01:26:05.42 +59:01:17.1: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 14.3988* 01 26 05.42 +59 01 17.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.5231+59.0209,2461174.8988,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.5231+59.0209 20260514.3988 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.99 02:00:32.76 +59:40:06.9
131.56327 -2.04003 galactic Cas Second-epoch detections are separated by 0.8" and 6.2 pix
The object was found in VSX 3" ZTF J020033.07+594008.7
Type: SR
# Max. Min./Amp. JD0 Period
13.621 r Y 0.477 r 2458342.93970 344.838134100000 C
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 02:00:32.76 +59:40:06.9: 11.48 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.76 +59:40:06.9: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.81 +/- 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 14.3988* 02 00 32.76 +59 40 06.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J020033.07+594008.7,2461174.8988,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J020033.07+594008.7 20260514.3988 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.03 01:50:39.73 +62:00:57.4
129.81882 -0.06131 galactic Cas Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511356332360621440 | 01:50:34.89 +62:00:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1955ApJS....2..123F LF 5 +61 158 J-Ks=1.202+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.73 +62:00:57.4: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.73 +62:00:57.4: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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 14.3988* 01 50 39.73 +62 00 57.4 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511356332360621440,2461174.8988,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511356332360621440 20260514.3988 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 10.96 01:09:22.60 +57:26:32.8
125.35412 -5.34491 galactic Cas Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.3204+57.4562 | 01:09:17.29 +57:26:45.5 (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 01:09:22.60 +57:26:32.8: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.60 +57:26:32.8: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 09 22.60 +57 26 32.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.3204+57.4562,2461174.8988,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.3204+57.4562 20260514.3988 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.04 01:06:55.57 +59:18:57.8
124.91041 -3.49618 galactic Cas Second-epoch detections are separated by 3.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.57 +59:18:57.8 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.57 +59:18:57.8: 13.13 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.57 +59:18:57.8: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 06 55.57 +59 18 57.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.12 01:44:29.73 +65:09:24.8
128.47060 2.85727 galactic Cas Second-epoch detections are separated by 1.9" and 5.9 pix
The object was found in VSX 5" Gaia DR3 519045973088246784
Type: ROT
# Max. Min./Amp. JD0 Period
15.090 G 15.140 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:29.73 +65:09:24.8: 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 01:44:29.73 +65:09:24.8: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 14.3988* 01 44 29.73 +65 09 24.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 519045973088246784,2461174.8988,11.12,0.05,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 519045973088246784 20260514.3988 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 14.3988 2461174.8988 11.12 01:52:55.08 +59:33:32.4
130.65615 -2.38757 galactic Cas Second-epoch detections are separated by 0.6" and 6.1 pix
The object was found in VSX17" Gaia DR3 506553498077188608
Type: ROT
# Max. Min./Amp. JD0 Period
15.360 G 15.380 G 2.474540000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:55.08 +59:33:32.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:55.08 +59:33:32.4: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 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 14.3988* 01 52 55.08 +59 33 32.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506553498077188608,2461174.8988,11.12,0.05,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 506553498077188608 20260514.3988 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 14.3988 2461174.8988 11.11 02:00:35.52 +58:32:34.3
131.86723 -3.12404 galactic Cas Second-epoch detections are separated by 2.1" and 5.9 pix
The object was found in VSX 1" Gaia DR3 505514390872372096
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.810 G 13.850 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:35.52 +58:32:34.3: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:35.52 +58:32:34.3: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 14.3988* 02 00 35.52 +58 32 34.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505514390872372096,2461174.8988,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505514390872372096 20260514.3988 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.10 01:44:03.12 +61:54:45.2
129.08249 -0.32927 galactic Cas Second-epoch detections are separated by 2.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511486800591720192 | 01:44:01.89 +61:55:16.8 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B1V 1999A&AS..136..313S Cl* NGC 654 Sto 94
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:03.12 +61:54:45.2: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:03.12 +61:54:45.2: 13.95 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.12
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 14.3988* 01 44 03.12 +61 54 45.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511486800591720192,2461174.8988,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511486800591720192 20260514.3988 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.24 01:33:30.60 +58:02:24.7
128.49306 -4.37656 galactic Cas Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.3712+58.0394 | 01:33:30.60 +58:02:24.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.820+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:30.60 +58:02:24.7: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:30.60 +58:02:24.7: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 14.3988* 01 33 30.60 +58 02 24.7 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.3712+58.0394,2461174.8988,11.24,0.05,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
ATO J023.3712+58.0394 20260514.3988 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 14.3988 2461174.8988 11.06 01:58:14.13 +60:03:14.6
131.18274 -1.74329 galactic Cas Second-epoch detections are separated by 1.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:58:14.13 +60:03:14.6 (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 01:58:14.13 +60:03:14.6: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:14.13 +60:03:14.6: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.99 +/- 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 14.3988* 01 58 14.13 +60 03 14.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.18 02:11:59.64 +63:23:15.5
131.80902 1.91281 galactic Cas Second-epoch detections are separated by 1.4" and 6.4 pix
The object was found in VSX14" ZTF J021201.47+632309.0
Type: EW
# Max. Min./Amp. JD0 Period
19.319 r Y 0.453 r 2458289.97240 0.293789200000
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 02:11:59.64 +63:23:15.5: 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 02:11:59.64 +63:23:15.5: 14.26 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 02 11 59.64 +63 23 15.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J021201.47+632309.0,2461174.8988,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J021201.47+632309.0 20260514.3988 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.13 02:15:10.46 +58:07:02.8
133.82458 -2.97237 galactic Per Second-epoch detections are separated by 1.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J033.7918+58.1304 | 02:15:08.45 +58:07:26.7 (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 02:15:10.46 +58:07:02.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:10.46 +58:07:02.8: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 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 14.3988* 02 15 10.46 +58 07 02.8 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
ATO J033.7918+58.1304,2461174.8988,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J033.7918+58.1304 20260514.3988 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.19 01:51:53.34 +63:26:20.5
129.62861 1.35599 galactic Cas Second-epoch detections are separated by 0.9" and 6.0 pix
The object was found in VSX 9" ZTF J015152.31+632614.6
Type: EB:
# Max. Min./Amp. JD0 Period
15.451 r Y 0.389 r 2458367.82620 5.408679200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:53.34 +63:26:20.5: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:53.34 +63:26:20.5: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 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 14.3988* 01 51 53.34 +63 26 20.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J015152.31+632614.6,2461174.8988,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J015152.31+632614.6 20260514.3988 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.27 02:02:11.31 +61:55:32.4
131.15265 0.18842 galactic Cas Second-epoch detections are separated by 3.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:02:11.31 +61:55:32.4 (user input) | T | P | (position from user input) J-Ks=0.538+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:11.31 +61:55:32.4: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:11.31 +61:55:32.4: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 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 14.3988* 02 02 11.31 +61 55 32.4 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260514.3988 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.29 01:51:39.96 +60:56:18.3
130.18259 -1.08263 galactic Cas Second-epoch detections are separated by 3.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 508195305151165312 | 01:51:34.71 +60:55:58.1 (Gaia DR3) | ROT (local) | (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 01:51:39.96 +60:56:18.3: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:39.96 +60:56:18.3: 14.12 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 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 14.3988* 01 51 39.96 +60 56 18.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508195305151165312,2461174.8988,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508195305151165312 20260514.3988 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.20 01:27:12.00 +57:43:01.1
127.71015 -4.82262 galactic Cas Second-epoch detections are separated by 2.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.7915+57.7249 | 01:27:12.00 +57:43:01.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:12.00 +57:43:01.1: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:12.00 +57:43:01.1: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 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 14.3988* 01 27 12.00 +57 43 01.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.7915+57.7249,2461174.8988,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.7915+57.7249 20260514.3988 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.21 01:26:28.44 +59:41:36.2
127.34468 -2.87784 galactic Cas Second-epoch detections are separated by 1.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.6536+59.6928 | 01:26:31.85 +59:41:21.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:28.44 +59:41:36.2: 12.91 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:28.44 +59:41:36.2: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 14.3988* 01 26 28.44 +59 41 36.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.6536+59.6928,2461174.8988,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.6536+59.6928 20260514.3988 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.36 01:44:33.16 +60:39:32.7
129.39650 -1.54427 galactic Cas Second-epoch detections are separated by 3.7" and 6.6 pix
The object was found in VSX20" Gaia DR3 509678172685830016
Type: ROT
# Max. Min./Amp. JD0 Period
16.410 G 16.450 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:33.16 +60:39:32.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:33.16 +60:39:32.7: 14.28 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.12
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 14.3988* 01 44 33.16 +60 39 32.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509678172685830016,2461174.8988,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509678172685830016 20260514.3988 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.29 02:16:55.73 +62:27:10.6
132.63714 1.20310 galactic Cas Second-epoch detections are separated by 5.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 513826320816760832 | 02:17:00.77 +62:27:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1978A&AS...32...25R BD+61 395
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:55.73 +62:27:10.6: 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 02:16:55.73 +62:27:10.6: 14.30 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 02 16 55.73 +62 27 10.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 513826320816760832,2461174.8988,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 513826320816760832 20260514.3988 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.22 02:15:03.60 +58:28:56.8
133.69406 -2.63112 galactic Per Second-epoch detections are separated by 4.8" and 7.0 pix
The object was found in VSX 5" Gaia DR3 506806798067617152
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.780 G 13.810 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 02:15:03.60 +58:28:56.8: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:03.60 +58:28:56.8: 13.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 14.3988* 02 15 03.60 +58 28 56.8 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 506806798067617152,2461174.8988,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506806798067617152 20260514.3988 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.46 01:31:36.06 +61:55:28.4
127.63883 -0.57959 galactic Cas Second-epoch detections are separated by 1.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510792527721618176 | 01:31:32.01 +61:55:56.5 (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 01:31:36.06 +61:55:28.4: 12.88 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:36.06 +61:55:28.4: 14.51 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.09
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 14.3988* 01 31 36.06 +61 55 28.4 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510792527721618176,2461174.8988,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510792527721618176 20260514.3988 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.29 02:02:25.11 +64:38:26.8
130.44158 2.80897 galactic Cas Second-epoch detections are separated by 6.9" and 6.6 pix
The object was found in VSX 7" ASASSN-V J020225.96+643822.9
Type: SR
# Max. Min./Amp. JD0 Period
14.090 V 14.200 V 2457555.11300 70.630000000000
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 02:02:25.11 +64:38:26.8: 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 02:02:25.11 +64:38:26.8: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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 14.3988* 02 02 25.11 +64 38 26.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020225.96+643822.9,2461174.8988,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J020225.96+643822.9 20260514.3988 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.42 01:51:52.42 +60:27:45.4
130.31756 -1.53961 galactic Cas Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:51:52.42 +60:27:45.4 (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 01:51:52.42 +60:27:45.4: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:52.42 +60:27:45.4: 14.32 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 51 52.42 +60 27 45.4 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.42,0.05,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 20260514.3988 11.42CV 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 14.3988 2461174.8988 11.59 01:21:23.76 +62:18:34.2
126.40455 -0.36008 galactic Cas Second-epoch detections are separated by 2.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510994391181101440 | 01:21:22.41 +62:19:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9 1935BSD...C01....0S BSD 8-1812
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:23.76 +62:18:34.2: 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 01:21:23.76 +62:18:34.2: 14.54 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 21 23.76 +62 18 34.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510994391181101440,2461174.8988,11.59,0.05,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 510994391181101440 20260514.3988 11.59CV 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 14.3988 2461174.8988 11.53 01:21:35.25 +61:01:27.0
126.57675 -1.63404 galactic Cas Second-epoch detections are separated by 1.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510493769787209600 | 01:21:35.66 +61:00:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1960IzKry..24..160B [B60] +60 169 J-Ks=0.488+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:35.25 +61:01:27.0: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:35.25 +61:01:27.0: 14.58 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.10
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 14.3988* 01 21 35.25 +61 01 27.0 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510493769787209600,2461174.8988,11.53,0.05,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 510493769787209600 20260514.3988 11.53CV 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 14.3988 2461174.8988 11.46 01:55:15.05 +58:45:59.4
131.13750 -3.08489 galactic Cas Second-epoch detections are separated by 2.9" and 5.7 pix
The object was found in VSX 4" Gaia DR3 506265151151611264
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.350 G 14.390 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 01:55:15.05 +58:45:59.4: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:15.05 +58:45:59.4: 14.33 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 55 15.05 +58 45 59.4 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506265151151611264,2461174.8988,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506265151151611264 20260514.3988 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.61 01:21:59.07 +62:31:56.3
126.44610 -0.13083 galactic Cas Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:21:59.07 +62:31:56.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:59.07 +62:31:56.3: 12.30 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:59.07 +62:31:56.3: 14.46 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 21 59.07 +62 31 56.3 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461174.8988,11.61,0.05,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 20260514.3988 11.61CV 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 14.3988 2461174.8988 11.71 01:28:14.69 +60:19:22.3
127.47643 -2.22371 galactic Cas Second-epoch detections are separated by 1.9" and 6.1 pix
The object was found in VSX15" Gaia DR3 510216005670888320
Type: ROT
# Max. Min./Amp. JD0 Period
17.120 G 17.200 G 3.707550000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:14.69 +60:19:22.3: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:14.69 +60:19:22.3: 14.68 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 14.3988* 01 28 14.69 +60 19 22.3 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510216005670888320,2461174.8988,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510216005670888320 20260514.3988 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 14.3988 2461174.8988 11.80 01:52:07.79 +59:53:02.5
130.48319 -2.09492 galactic Cas Second-epoch detections are separated by 2.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 506579645838190208 | 01:52:03.18 +59:52:32.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: B2 1953IzKry..10..120K [K53] 612
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:07.79 +59:53:02.5: 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 01:52:07.79 +59:53:02.5: 14.67 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.10
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 14.3988* 01 52 07.79 +59 53 02.5 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 506579645838190208,2461174.8988,11.80,0.05,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
Large-amplitude variable Gaia DR2 506579645838190208 20260514.3988 11.80CV 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
## 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: 2461174.89905404 14.05.2026 09:34:28.269 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
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: 41 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): 26463
Objects passed selection criteria: 26333
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 19419.2
Average stars matched: 17712.8 (91.2123 %)
Memory usage VmPeak: 128288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 14 05:27:40 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: 2461174.89905404 14.05.2026 09:34:28.269 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 190
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: 228 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): 190094
Objects passed selection criteria: 189605
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 144716
Average stars matched: 132430 (91.5098 %)
Memory usage VmPeak: 1944212 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 14 05:38:58 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_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.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_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.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: 2461174.89858904
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_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.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_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
Image size: 938.8'x624.3' 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: 01:42:41.644 +62:00:24.24 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 01:42:41.644 +62:00:24.24
Angular distance between the image centers 0.0333 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
Image size: 938.8'x624.3' 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: 01:42:42.479 +61:59:48.40 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 01:42:42.479 +61:59:48.40
Angular distance between the image centers 0.0294 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 01:42:41.644 +62:00:24.24
Second-epoch second image center 01:42:42.479 +61:59:48.40
Angular distance between the image centers 0.01009 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.MJ5MUlM8kv
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.lAq1LsXd1V
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_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits &> /tmp/tmp.Coj537y7pV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits &> /tmp/tmp.qBwGFzyCvc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.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 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.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
14.6 mag. fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
14.6 mag. fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.8 (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.MJ5MUlM8kv (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_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/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)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=331 sigma_overall_arcsec=7.729 sigma_q1_arcsec=31.346 sigma_q2_arcsec=12.794 sigma_q3_arcsec=22.422 sigma_q4_arcsec=4.202 n_q1=16 n_q2=97 n_q3=37 n_q4=181 worst_quadrant_to_overall_ratio=4.055
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.lAq1LsXd1V (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_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/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! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=973 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.346 n_q1=119 n_q2=244 n_q3=303 n_q4=307 worst_quadrant_to_overall_ratio=1.316
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.Coj537y7pV (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_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.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_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.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_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1549, passed=19191
Got 19191 stars (including 17628 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 19191 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 18801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 18797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 18797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 974 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits N_match=974 sigma_overall_arcsec=0.662 sigma_q1_arcsec=0.579 sigma_q2_arcsec=0.635 sigma_q3_arcsec=0.690 sigma_q4_arcsec=0.665 n_q1=257 n_q2=340 n_q3=212 n_q4=165 worst_quadrant_to_overall_ratio=1.042
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.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.qBwGFzyCvc (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_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.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_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.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_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1570, passed=19166
Got 19166 stars (including 17588 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits.cat
util/solve_plate_with_UCAC5 got 19166 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 18762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 975 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(), 18759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 18759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits N_match=974 sigma_overall_arcsec=0.621 sigma_q1_arcsec=0.574 sigma_q2_arcsec=0.593 sigma_q3_arcsec=0.699 sigma_q4_arcsec=0.675 n_q1=257 n_q2=342 n_q3=207 n_q4=168 worst_quadrant_to_overall_ratio=1.126
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=7.729 worst_q_ratio=4.055
ref2=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.405 worst_q_ratio=1.316
new1=fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits sigma_overall=0.662 worst_q_ratio=1.042
new2=fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits sigma_overall=0.621 worst_q_ratio=1.126
reference average sigma_overall=4.067 worst_q_ratio=2.6855
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (331 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (973 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229_astrometric_residuals.png (974 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230_astrometric_residuals.png (974 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-33-48_20.00sec_-4.90C_LIGHT_0229.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-14_CI_Cas-03-Q2b1x1_052228_TTUQ2b1x1_3120439_yJ0V2ZJL/wcs_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:06.21 +63:57:56.9: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:11.29 +58:01:03.7: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:06.21 +63:57:56.9: 12.29 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:11.29 +58:01:03.7: 10.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry reference-image weighted average: 10.64 +/- 0.00
Forced photometry filter REJECTED candidate at 01:55:06.21 +63:57:56.9: ref_mag=12.29 +/- 0.01 new_mean_mag=12.1132 delta=0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:09:11.29 +58:01:03.7: ref_mag=10.64 +/- 0.00 new_mean_mag=10.8359 delta=-0.20 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 2s
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
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Considering the candidate 51604_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 51604_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
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Considering the candidate 55106_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 55106_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:46:08.55 +61:12:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56219_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 56219_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:11:03.57 +57:20:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56343_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 56343_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
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Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 08339_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
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Considering the candidate 247630_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247630_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247640_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247640_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247645_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247645_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247659_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247659_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Successfully moved fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.png to transient_report/247659_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230_discovery2.png
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Considering the candidate 247666_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247666_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247667_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247667_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247678_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247678_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247680_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247680_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247681_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247681_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247685_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247685_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247691_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247691_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247697_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247697_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247698_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247698_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 247699_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247699_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247703_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247703_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247706_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247706_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247708_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247708_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247709_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247709_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
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Considering the candidate 247711_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247711_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:30:06.59 +61:51:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247712_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247712_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247720_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247720_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247722_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247722_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247725_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247725_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247726_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247726_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247727_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247727_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247728_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247728_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247730_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247730_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247732_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247732_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247733_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247733_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247735_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247735_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247737_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247737_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247739_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247739_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247740_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247740_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:50:44.96 +58:00:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247741_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247741_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:13:31.04 +65:37:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 5.508 515599901791080320 033.37658693287 +65.61669477337 11.7314 10.1460 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247745_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247745_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247749_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247749_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:12:31.06 +61:17:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247755_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247755_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
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Considering the candidate 247756_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247756_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247757_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247757_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:33:01.28 +59:16:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247762_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247762_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247764_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247764_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247765_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247765_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247768_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247768_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:07:35.08 +57:33:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247769_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247769_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
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Considering the candidate 247771_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247771_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:33:35.27 +59:56:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247772_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247772_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247773_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247773_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:07:33.85 +60:52:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247774_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247774_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247778_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247778_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247783_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247783_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:39:04.14 +61:53:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247784_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247784_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:14:45.22 +60:30:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247787_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247787_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 247791_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247791_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:07:08.09 +57:44:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247793_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247793_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:43:59.19 +61:55:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247794_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247794_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:55:14.54 +59:32:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247795_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247795_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:15:16.80 +57:28:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247796_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 247796_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 247803_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247803_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:51:35.68 +57:52:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247804_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 247804_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:22:08.27 +60:22:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251580_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 251580_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:44:02.07 +61:53:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252197_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 252197_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:19:11.06 +58:20:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252621_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 252621_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:38:00.37 +57:56:47.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253679_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 253679_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:26:41.05 +60:46:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254424_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 254424_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:28:15.30 +58:44:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256927_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 256927_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:43:52.96 +61:53:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257354_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 257354_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:44:17.70 +61:53:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257725_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 257725_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:16:04.84 +58:49:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258225_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 258225_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:15:58.82 +63:12:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259109_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 259109_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:02:54.73 +64:25:00.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259963_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 259963_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:11:23.04 +61:21:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260037_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 260037_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:00:36.86 +58:30:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260192_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 260192_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:11:50.26 +59:02:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260526_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 260526_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:26:35.87 +57:57:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260551_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 260551_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:13:30.00 +58:34:26.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 260975_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 260975_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:04:26.62 +65:05:54.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261125_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 261125_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:34:10.20 +62:09:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261331_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 261331_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:06:23.38 +62:44:06.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261681_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 261681_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:19:03.70 +63:57:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261814_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 261814_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:58:04.17 +57:58:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262027_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 262027_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:33:23.09 +57:44:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262289_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 262289_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:10:23.80 +60:01:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262650_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 262650_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 262828_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 262828_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:01:14.93 +59:23:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263353_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 263353_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:59:05.82 +59:55:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263500_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 263500_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:19:41.57 +62:51:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263693_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 263693_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:08:30.66 +58:24:20.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 264301_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 264301_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:48:39.77 +59:09:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264705_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 264705_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:37:13.81 +58:38:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264904_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 264904_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:42:54.79 +64:01:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265096_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 265096_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:37:13.65 +58:38:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265183_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 265183_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:38:11.99 +61:01:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265397_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 265397_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:44:56.53 +59:46:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265513_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 265513_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:16:36.99 +64:56:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265551_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 265551_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:38:06.30 +58:10:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265595_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 265595_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:23:07.48 +61:11:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265599_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 265599_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 265790_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 265790_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:02:53.91 +60:15:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265835_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 265835_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:18:04.19 +65:36:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265864_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 265864_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:37:41.39 +58:37:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266128_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 266128_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:46:18.06 +60:59:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266174_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 266174_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 266341_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 266341_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:27:56.32 +62:46:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266399_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 266399_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:14:00.26 +61:42:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266608_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 266608_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266715_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 266715_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:44:32.33 +61:36:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266758_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 266758_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:42:28.22 +58:17:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266777_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 266777_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:14:00.56 +59:02:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266829_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 266829_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 266871_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 266871_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:34:42.54 +58:42:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266949_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 266949_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 267029_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 267029_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:43:03.23 +58:57:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267153_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 267153_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:56:25.29 +62:05:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267213_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 267213_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 267327_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 267327_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 267746_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 267746_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:49:06.12 +65:23:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267918_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 267918_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:27:04.14 +64:43:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267950_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 267950_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:54:30.16 +59:06:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267985_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 267985_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 268005_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 268005_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 268040_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 268040_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:34:34.58 +65:48:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268266_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 268266_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:54:06.37 +61:05:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268337_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 268337_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268458_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 268458_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:10:10.22 +59:08:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269168_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 269168_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:03:25.16 +57:50:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269446_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 269446_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:55:05.05 +59:57:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269603_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 269603_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 269814_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 269814_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:42:49.45 +61:24:06.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 269887_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 269887_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 269923_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 269923_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 270221_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 270221_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 270347_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 270347_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 270661_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 270661_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 270675_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 270675_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:37:55.45 +58:09:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271106_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 271106_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 271108_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 271108_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 271115_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 271115_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 271403_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 271403_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 271505_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 271505_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 271611_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 271611_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 271839_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 271839_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:48:34.98 +58:41:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272189_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 272189_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 272242_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 272242_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 272492_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 272492_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 272550_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 272550_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 273557_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 273557_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 273668_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 273668_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 274049_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 274049_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 274055_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 274055_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 274246_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 274246_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Successfully moved fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230.png to transient_report/274246_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230_discovery2.png
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Considering the candidate 274255_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 274255_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 274534_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 274534_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 275029_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 275029_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 275121_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 275121_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:13:35.39 +58:31:50.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 275239_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 275239_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
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Considering the candidate 275463_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 275463_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 275702_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 275702_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:48:21.34 +62:53:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 277066_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 277066_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 277345_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 277345_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
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Considering the candidate 277656_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
Preparing report for the candidate 277656_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
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Considering the candidate 234396_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 234396_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:29:32.90 +63:18:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 112593_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:21:55.29 +61:21:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 72532_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:45:35.50 +63:07:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 70271_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 02:20:32.49 +62:32:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34158_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 34158_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:39:32.43 +64:53:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230
The candidate 39378_fd_Cas-03-Q2b1x1_2026-05-14_04-34-28_20.00sec_-4.90C_LIGHT_0230 did not pass the final checks
**** FOUND 01:47:55.58 +64:32:56.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 19s
make_report_in_HTML.sh TOTAL: 253s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:58:29.33 +63:45:09.2
01:55:28.41 +63:18:58.4
01:26:31.82 +61:19:28.1
01:28:22.63 +57:57:58.8
01:41:51.95 +60:08:24.8
01:37:23.78 +59:20:13.2
01:11:19.87 +61:17:56.6
01:33:12.70 +61:16:56.9
01:19:46.43 +63:03:13.4
01:54:24.55 +61:25:41.9
01:16:38.51 +63:11:33.2
01:12:41.30 +61:18:09.6
01:05:42.77 +62:52:34.3
01:08:39.10 +60:32:42.8
01:13:01.38 +61:01:00.6
01:38:38.44 +61:15:26.1
01:12:09.70 +58:47:54.8
01:07:36.78 +58:09:26.4
01:25:27.50 +59:27:17.3
01:47:51.38 +61:11:14.0
01:35:41.55 +61:13:14.2
01:10:03.10 +57:48:14.8
01:10:11.76 +59:17:25.9
01:20:42.36 +66:02:08.4
01:51:47.25 +58:37:59.8
01:15:44.74 +60:02:47.1
01:29:02.54 +58:46:11.6
01:05:20.99 +64:15:24.0
01:07:39.23 +59:59:20.2
01:24:54.95 +59:41:48.8
02:06:09.31 +62:45:45.0
01:09:21.52 +64:35:19.4
01:26:36.61 +59:41:36.1
01:11:44.58 +61:13:58.7
01:07:31.53 +61:28:29.3
01:08:23.16 +61:35:11.1
01:38:10.70 +60:44:57.0
01:20:24.32 +59:10:25.8
01:29:33.67 +63:19:32.1
01:18:48.42 +64:12:23.7
01:11:56.58 +58:41:06.3
01:31:48.39 +64:22:29.0
01:38:34.53 +57:58:02.8
01:13:38.83 +58:10:53.0
01:26:05.42 +59:01:17.1
02:00:32.76 +59:40:06.9
01:50:39.73 +62:00:57.4
01:09:22.60 +57:26:32.8
01:06:55.57 +59:18:57.8
01:44:29.73 +65:09:24.8
01:52:55.08 +59:33:32.4
02:00:35.52 +58:32:34.3
01:44:03.12 +61:54:45.2
01:33:30.60 +58:02:24.7
01:58:14.13 +60:03:14.6
02:11:59.64 +63:23:15.5
02:15:10.46 +58:07:02.8
01:51:53.34 +63:26:20.5
02:02:11.31 +61:55:32.4
01:51:39.96 +60:56:18.3
01:27:12.00 +57:43:01.1
01:26:28.44 +59:41:36.2
01:44:33.16 +60:39:32.7
02:16:55.73 +62:27:10.6
02:15:03.60 +58:28:56.8
01:31:36.06 +61:55:28.4
02:02:25.11 +64:38:26.8
01:51:52.42 +60:27:45.4
01:21:23.76 +62:18:34.2
01:21:35.25 +61:01:27.0
01:55:15.05 +58:45:59.4
01:21:59.07 +62:31:56.3
01:28:14.69 +60:19:22.3
01:52:07.79 +59:53:02.5
########### 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 ####
01:58:29.33 +63:45:09.2
01:55:28.41 +63:18:58.4
01:26:31.82 +61:19:28.1
01:28:22.63 +57:57:58.8
01:41:51.95 +60:08:24.8
01:37:23.78 +59:20:13.2
01:11:19.87 +61:17:56.6
01:33:12.70 +61:16:56.9
01:19:46.43 +63:03:13.4
01:54:24.55 +61:25:41.9
01:16:38.51 +63:11:33.2
01:12:41.30 +61:18:09.6
01:05:42.77 +62:52:34.3
01:08:39.10 +60:32:42.8
01:13:01.38 +61:01:00.6
01:38:38.44 +61:15:26.1
01:12:09.70 +58:47:54.8
01:07:36.78 +58:09:26.4
01:25:27.50 +59:27:17.3
01:47:51.38 +61:11:14.0
01:35:41.55 +61:13:14.2
01:10:03.10 +57:48:14.8
01:10:11.76 +59:17:25.9
01:20:42.36 +66:02:08.4
01:51:47.25 +58:37:59.8
01:15:44.74 +60:02:47.1
01:29:02.54 +58:46:11.6
01:05:20.99 +64:15:24.0
01:07:39.23 +59:59:20.2
01:24:54.95 +59:41:48.8
02:06:09.31 +62:45:45.0
01:09:21.52 +64:35:19.4
01:26:36.61 +59:41:36.1
01:11:44.58 +61:13:58.7
01:07:31.53 +61:28:29.3
01:08:23.16 +61:35:11.1
01:38:10.70 +60:44:57.0
01:20:24.32 +59:10:25.8
01:29:33.67 +63:19:32.1
01:18:48.42 +64:12:23.7
01:11:56.58 +58:41:06.3
01:31:48.39 +64:22:29.0
01:38:34.53 +57:58:02.8
01:13:38.83 +58:10:53.0
01:26:05.42 +59:01:17.1
02:00:32.76 +59:40:06.9
01:50:39.73 +62:00:57.4
01:09:22.60 +57:26:32.8
01:06:55.57 +59:18:57.8
01:44:29.73 +65:09:24.8
01:52:55.08 +59:33:32.4
02:00:35.52 +58:32:34.3
01:44:03.12 +61:54:45.2
01:33:30.60 +58:02:24.7
01:58:14.13 +60:03:14.6
02:11:59.64 +63:23:15.5
02:15:10.46 +58:07:02.8
01:51:53.34 +63:26:20.5
02:02:11.31 +61:55:32.4
01:51:39.96 +60:56:18.3
01:27:12.00 +57:43:01.1
01:26:28.44 +59:41:36.2
01:44:33.16 +60:39:32.7
02:16:55.73 +62:27:10.6
02:15:03.60 +58:28:56.8
01:31:36.06 +61:55:28.4
02:02:25.11 +64:38:26.8
01:51:52.42 +60:27:45.4
01:21:23.76 +62:18:34.2
01:21:35.25 +61:01:27.0
01:55:15.05 +58:45:59.4
01:21:59.07 +62:31:56.3
01:28:14.69 +60:19:22.3
01:52:07.79 +59:53:02.5
###################################################################################
01:58:29.33 +63:45:09.2 -- not an asteroid (will add it to exclusion list)
01:55:28.41 +63:18:58.4 -- not an asteroid (will add it to exclusion list)
01:26:31.82 +61:19:28.1 -- not an asteroid (will add it to exclusion list)
01:28:22.63 +57:57:58.8 -- not an asteroid (will add it to exclusion list)
01:41:51.95 +60:08:24.8 -- not an asteroid (will add it to exclusion list)
01:37:23.78 +59:20:13.2 -- not an asteroid (will add it to exclusion list)
01:11:19.87 +61:17:56.6 -- not an asteroid (will add it to exclusion list)
01:33:12.70 +61:16:56.9 -- not an asteroid (will add it to exclusion list)
01:19:46.43 +63:03:13.4 -- not an asteroid (will add it to exclusion list)
01:54:24.55 +61:25:41.9 -- not an asteroid (will add it to exclusion list)
01:16:38.51 +63:11:33.2 -- not an asteroid (will add it to exclusion list)
01:12:41.30 +61:18:09.6 -- not an asteroid (will add it to exclusion list)
01:05:42.77 +62:52:34.3 -- not an asteroid (will add it to exclusion list)
01:08:39.10 +60:32:42.8 -- not an asteroid (will add it to exclusion list)
01:13:01.38 +61:01:00.6 -- not an asteroid (will add it to exclusion list)
01:38:38.44 +61:15:26.1 -- not an asteroid (will add it to exclusion list)
01:12:09.70 +58:47:54.8 -- not an asteroid (will add it to exclusion list)
01:07:36.78 +58:09:26.4 -- not an asteroid (will add it to exclusion list)
01:25:27.50 +59:27:17.3 -- not an asteroid (will add it to exclusion list)
01:47:51.38 +61:11:14.0 -- not an asteroid (will add it to exclusion list)
01:35:41.55 +61:13:14.2 -- not an asteroid (will add it to exclusion list)
01:10:03.10 +57:48:14.8 -- not an asteroid (will add it to exclusion list)
01:10:11.76 +59:17:25.9 -- not an asteroid (will add it to exclusion list)
01:20:42.36 +66:02:08.4 -- not an asteroid (will add it to exclusion list)
01:51:47.25 +58:37:59.8 -- not an asteroid (will add it to exclusion list)
01:15:44.74 +60:02:47.1 -- not an asteroid (will add it to exclusion list)
01:29:02.54 +58:46:11.6 -- not an asteroid (will add it to exclusion list)
01:05:20.99 +64:15:24.0 -- not an asteroid (will add it to exclusion list)
01:07:39.23 +59:59:20.2 -- not an asteroid (will add it to exclusion list)
01:24:54.95 +59:41:48.8 -- not an asteroid (will add it to exclusion list)
02:06:09.31 +62:45:45.0 -- not an asteroid (will add it to exclusion list)
01:09:21.52 +64:35:19.4 -- not an asteroid (will add it to exclusion list)
01:26:36.61 +59:41:36.1 -- not an asteroid (will add it to exclusion list)
01:11:44.58 +61:13:58.7 -- not an asteroid (will add it to exclusion list)
01:07:31.53 +61:28:29.3 -- not an asteroid (will add it to exclusion list)
01:08:23.16 +61:35:11.1 -- not an asteroid (will add it to exclusion list)
01:38:10.70 +60:44:57.0 -- not an asteroid (will add it to exclusion list)
01:20:24.32 +59:10:25.8 -- not an asteroid (will add it to exclusion list)
01:29:33.67 +63:19:32.1 -- not an asteroid (will add it to exclusion list)
01:18:48.42 +64:12:23.7 -- not an asteroid (will add it to exclusion list)
01:11:56.58 +58:41:06.3 -- not an asteroid (will add it to exclusion list)
01:31:48.39 +64:22:29.0 -- not an asteroid (will add it to exclusion list)
01:38:34.53 +57:58:02.8 -- not an asteroid (will add it to exclusion list)
01:13:38.83 +58:10:53.0 -- not an asteroid (will add it to exclusion list)
01:26:05.42 +59:01:17.1 -- not an asteroid (will add it to exclusion list)
02:00:32.76 +59:40:06.9 -- not an asteroid (will add it to exclusion list)
01:50:39.73 +62:00:57.4 -- not an asteroid (will add it to exclusion list)
01:09:22.60 +57:26:32.8 -- not an asteroid (will add it to exclusion list)
01:06:55.57 +59:18:57.8 -- not an asteroid (will add it to exclusion list)
01:44:29.73 +65:09:24.8 -- not an asteroid (will add it to exclusion list)
01:52:55.08 +59:33:32.4 -- not an asteroid (will add it to exclusion list)
02:00:35.52 +58:32:34.3 -- not an asteroid (will add it to exclusion list)
01:44:03.12 +61:54:45.2 -- not an asteroid (will add it to exclusion list)
01:33:30.60 +58:02:24.7 -- not an asteroid (will add it to exclusion list)
01:58:14.13 +60:03:14.6 -- not an asteroid (will add it to exclusion list)
02:11:59.64 +63:23:15.5 -- not an asteroid (will add it to exclusion list)
02:15:10.46 +58:07:02.8 -- not an asteroid (will add it to exclusion list)
01:51:53.34 +63:26:20.5 -- not an asteroid (will add it to exclusion list)
02:02:11.31 +61:55:32.4 -- not an asteroid (will add it to exclusion list)
01:51:39.96 +60:56:18.3 -- not an asteroid (will add it to exclusion list)
01:27:12.00 +57:43:01.1 -- not an asteroid (will add it to exclusion list)
01:26:28.44 +59:41:36.2 -- not an asteroid (will add it to exclusion list)
01:44:33.16 +60:39:32.7 -- not an asteroid (will add it to exclusion list)
02:16:55.73 +62:27:10.6 -- not an asteroid (will add it to exclusion list)
02:15:03.60 +58:28:56.8 -- not an asteroid (will add it to exclusion list)
01:31:36.06 +61:55:28.4 -- not an asteroid (will add it to exclusion list)
02:02:25.11 +64:38:26.8 -- not an asteroid (will add it to exclusion list)
01:51:52.42 +60:27:45.4 -- not an asteroid (will add it to exclusion list)
01:21:23.76 +62:18:34.2 -- not an asteroid (will add it to exclusion list)
01:21:35.25 +61:01:27.0 -- not an asteroid (will add it to exclusion list)
01:55:15.05 +58:45:59.4 -- not an asteroid (will add it to exclusion list)
01:21:59.07 +62:31:56.3 -- not an asteroid (will add it to exclusion list)
01:28:14.69 +60:19:22.3 -- not an asteroid (will add it to exclusion list)
01:52:07.79 +59:53:02.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:05:20.99 +64:15:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:42.77 +62:52:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.57 +59:18:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:31.53 +61:28:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:36.78 +58:09:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.23 +59:59:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:23.16 +61:35:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:39.10 +60:32:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:21.52 +64:35:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.60 +57:26:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:03.10 +57:48:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:11.76 +59:17:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:19.87 +61:17:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:44.58 +61:13:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:56.58 +58:41:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:09.70 +58:47:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:41.30 +61:18:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:01.38 +61:01:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:38.83 +58:10:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:44.74 +60:02:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:38.51 +63:11:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:48.42 +64:12:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:46.43 +63:03:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:24.32 +59:10:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:42.36 +66:02:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:23.76 +62:18:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:35.25 +61:01:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:59.07 +62:31:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:54.95 +59:41:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:27.50 +59:27:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.42 +59:01:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:28.44 +59:41:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:31.82 +61:19:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:36.61 +59:41:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:12.00 +57:43:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:14.69 +60:19:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:22.63 +57:57:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:02.54 +58:46:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:33.67 +63:19:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:36.06 +61:55:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.39 +64:22:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:12.70 +61:16:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:30.60 +58:02:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:41.55 +61:13:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:23.78 +59:20:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:10.70 +60:44:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:34.53 +57:58:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:38.44 +61:15:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:51.95 +60:08:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:03.12 +61:54:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:29.73 +65:09:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:33.16 +60:39:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:51.38 +61:11:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:39.73 +62:00:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:39.96 +60:56:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:47.25 +58:37:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:52.42 +60:27:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:53.34 +63:26:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:07.79 +59:53:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:55.08 +59:33:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:24.55 +61:25:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:15.05 +58:45:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:28.41 +63:18:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:14.13 +60:03:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:29.33 +63:45:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.76 +59:40:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:35.52 +58:32:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:11.31 +61:55:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:25.11 +64:38:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:09.31 +62:45:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:59.64 +63:23:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:03.60 +58:28:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:10.46 +58:07:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:55.73 +62:27:10.6 -- 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)
01:05:20.99 +64:15:24.0 -- not a known variable star
01:05:42.77 +62:52:34.3 -- not a known variable star
01:06:55.57 +59:18:57.8 -- not a known variable star
01:07:31.53 +61:28:29.3 -- not a known variable star
01:07:36.78 +58:09:26.4 -- not a known variable star
01:07:39.23 +59:59:20.2 -- not a known variable star
01:08:23.16 +61:35:11.1 -- not a known variable star
01:08:39.10 +60:32:42.8 -- not a known variable star
01:09:21.52 +64:35:19.4 -- not a known variable star
01:09:22.60 +57:26:32.8 -- not a known variable star
01:10:03.10 +57:48:14.8 -- not a known variable star
01:10:11.76 +59:17:25.9 -- not a known variable star
01:11:19.87 +61:17:56.6 -- not a known variable star
01:11:44.58 +61:13:58.7 -- a known variable star
01:11:56.58 +58:41:06.3 -- not a known variable star
01:12:09.70 +58:47:54.8 -- not a known variable star
01:12:41.30 +61:18:09.6 -- not a known variable star
01:13:01.38 +61:01:00.6 -- a known variable star
01:13:38.83 +58:10:53.0 -- not a known variable star
01:15:44.74 +60:02:47.1 -- not a known variable star
01:16:38.51 +63:11:33.2 -- a known variable star
01:18:48.42 +64:12:23.7 -- not a known variable star
01:19:46.43 +63:03:13.4 -- not a known variable star
01:20:24.32 +59:10:25.8 -- not a known variable star
01:20:42.36 +66:02:08.4 -- not a known variable star
01:21:23.76 +62:18:34.2 -- not a known variable star
01:21:35.25 +61:01:27.0 -- not a known variable star
01:21:59.07 +62:31:56.3 -- not a known variable star
01:24:54.95 +59:41:48.8 -- not a known variable star
01:25:27.50 +59:27:17.3 -- a known variable star
01:26:05.42 +59:01:17.1 -- not a known variable star
01:26:28.44 +59:41:36.2 -- not a known variable star
01:26:31.82 +61:19:28.1 -- not a known variable star
01:26:36.61 +59:41:36.1 -- a known variable star
01:27:12.00 +57:43:01.1 -- not a known variable star
01:28:14.69 +60:19:22.3 -- a known variable star
01:28:22.63 +57:57:58.8 -- not a known variable star
01:29:02.54 +58:46:11.6 -- not a known variable star
01:29:33.67 +63:19:32.1 -- a known variable star
01:31:36.06 +61:55:28.4 -- not a known variable star
01:31:48.39 +64:22:29.0 -- not a known variable star
01:33:12.70 +61:16:56.9 -- not a known variable star
01:33:30.60 +58:02:24.7 -- not a known variable star
01:35:41.55 +61:13:14.2 -- not a known variable star
01:37:23.78 +59:20:13.2 -- not a known variable star
01:38:10.70 +60:44:57.0 -- not a known variable star
01:38:34.53 +57:58:02.8 -- not a known variable star
01:38:38.44 +61:15:26.1 -- not a known variable star
01:41:51.95 +60:08:24.8 -- not a known variable star
01:44:03.12 +61:54:45.2 -- not a known variable star
01:44:29.73 +65:09:24.8 -- a known variable star
01:44:33.16 +60:39:32.7 -- a known variable star
01:47:51.38 +61:11:14.0 -- not a known variable star
01:50:39.73 +62:00:57.4 -- not a known variable star
01:51:39.96 +60:56:18.3 -- not a known variable star
01:51:47.25 +58:37:59.8 -- not a known variable star
01:51:52.42 +60:27:45.4 -- not a known variable star
01:51:53.34 +63:26:20.5 -- a known variable star
01:52:07.79 +59:53:02.5 -- not a known variable star
01:52:55.08 +59:33:32.4 -- a known variable star
01:54:24.55 +61:25:41.9 -- not a known variable star
01:55:15.05 +58:45:59.4 -- a known variable star
01:55:28.41 +63:18:58.4 -- not a known variable star
01:58:14.13 +60:03:14.6 -- not a known variable star
01:58:29.33 +63:45:09.2 -- not a known variable star
02:00:32.76 +59:40:06.9 -- a known variable star
02:00:35.52 +58:32:34.3 -- a known variable star
02:02:11.31 +61:55:32.4 -- not a known variable star
02:02:25.11 +64:38:26.8 -- a known variable star
02:06:09.31 +62:45:45.0 -- not a known variable star
02:11:59.64 +63:23:15.5 -- a known variable star
02:15:03.60 +58:28:56.8 -- a known variable star
02:15:10.46 +58:07:02.8 -- not a known variable star
02:16:55.73 +62:27:10.6 -- not a known variable star
Found 57 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
74 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 74 (excluding asteroids and hot pixels, 57 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461174.89858904 -observatory V36
03:22:17.00 +18:37:41.5 Mercury (-2.5mag)
05:33:51.69 +24:44:24.8 Venus (-3.9mag)
01:38:22.40 +09:23:00.2 Mars (1.2mag)
07:29:17.41 +22:15:15.5 Jupiter (-1.9mag)
00:41:02.51 +02:01:06.5 Saturn (0.9mag)
03:54:12.33 +20:07:44.6 Uranus (5.8mag)
00:14:09.54 +00:05:10.4 Neptune (7.8mag)
20:34:12.43 -22:56:46.7 Pluto (14.5mag)
01:09:13.76 +10:13:37.3 Moon (-8.9mag)
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Positions of selected moons from JPL HORIZONS for JD(UT)2461174.89858904:
07:29:18.08 +22:15:16.2 Io (5.9mag)
07:29:19.68 +22:15:12.3 Europa (6.1mag)
07:29:36.10 +22:14:27.5 Ganymede (5.5mag)
07:29:05.23 +22:15:52.9 Callisto (6.7mag)
07:31:05.72 +21:53:14.5 Himalia (15.5mag)
07:29:18.35 +22:15:11.7 Thebe (16.4mag)
07:31:33.12 +22:19:09.8 Elara (17.4mag)
07:30:02.60 +22:40:19.4 Pasiphae (17.6mag)
07:36:49.88 +22:15:22.4 Carme (18.7mag)
00:41:14.35 +02:01:09.0 Titan (8.7mag)
00:41:07.33 +02:01:03.1 Rhea (10.0mag)
00:40:57.79 +01:59:24.3 Iapetus (11.4mag)
00:40:51.28 +02:01:14.4 Hyperion (14.7mag)
00:42:13.06 +02:06:29.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 14 05:27 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461174.89858904:
17:02:45.09 -30:17:28.2 JWST
18:45:53.20 +21:44:54.3 Chandra
09:15:15.36 -52:49:15.2 XMM-Newton
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461174.89858904 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
13:32:55.67 -28:12:13.6 14.6mag D/1884 O1 (Barnard)
06:17:18.80 +30:54:32.0 15.8mag D/1886 K1 (Brooks)
15:37:05.09 +00:39:40.5 14.8mag D/1895 Q1 (Swift)
05:09:21.04 +24:09:29.6 17.1mag D/1918 W1 (Schorr)
08:04:47.68 +23:59:51.7 17.7mag P/2009 WX51 (Catalina)
18:54:57.76 -30:43:57.9 13.7mag P/2010 H2 (Vales)
05:29:58.55 -68:33:45.0 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:40:20.29 +31:40:48.0 17.4mag C/2017 K2 (PANSTARRS)
17:24:04.31 +13:34:49.1 17.7mag C/2021 G2 (ATLAS)
23:14:44.93 +30:30:07.1 17.2mag C/2022 E2 (ATLAS)
05:03:27.87 +26:41:00.2 16.3mag C/2022 N2 (PANSTARRS)
09:14:09.88 +31:46:49.3 16.4mag C/2022 QE78 (ATLAS)
08:38:58.07 +02:24:53.4 17.5mag C/2022 R6 (PANSTARRS)
18:42:53.97 +20:36:42.9 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:29:28.21 -11:08:08.3 17.5mag P/2023 B1 (PANSTARRS)
09:00:03.11 -07:56:22.1 17.9mag C/2023 F3 (ATLAS)
22:13:47.37 +64:48:58.4 17.7mag C/2023 H5 (Lemmon)
18:41:05.04 -04:43:55.9 13.8mag C/2023 R1 (PANSTARRS)
15:13:57.49 +87:50:20.3 17.9mag C/2023 X2 (Lemmon)
06:40:03.56 +63:41:02.8 17.5mag C/2024 A1 (ATLAS)
06:07:15.12 +24:51:42.7 12.6mag C/2024 E1 (Wierzchos)
15:57:45.16 +10:43:55.5 17.3mag C/2024 G6 (ATLAS)
20:22:56.38 +23:32:45.2 14.3mag C/2024 J3 (ATLAS)
03:53:16.91 -18:31:25.8 16.2mag C/2024 T5 (ATLAS)
05:42:30.48 +39:03:10.3 17.8mag C/2025 J1 (Borisov)
12:05:07.87 +53:18:50.8 16.5mag C/2025 L1 (ATLAS)
05:50:48.95 -08:38:45.5 10.9mag C/2025 R3 (PANSTARRS)
12:43:34.59 +04:20:55.1 17.3mag C/2025 Y1 (ATLAS)
01:11:22.82 +41:14:01.5 15.4mag C/2026 B2 (Sun-Gao)
11:13:17.13 -14:57:12.7 16.1mag A/2026 E1
19:37:32.22 -08:19:03.4 10.1mag 10P/Tempel
14:26:20.99 -00:40:34.9 16.6mag 24P/Schaumasse
10:59:00.36 -00:54:44.2 15.8mag 29P/Schwassmann-Wachmann
10:44:27.86 -02:40:22.1 17.5mag 43P/Wolf-Harrington
02:33:00.29 +22:05:11.4 17.5mag 47P/Ashbrook-Jackson
08:07:22.40 +30:25:22.5 16.9mag 63P/Wild
00:02:40.09 -08:22:04.8 15.7mag 65P/Gunn
05:24:54.05 +29:22:44.6 16.3mag 76P/West-Kohoutek-Ikemura
02:10:10.95 +13:29:17.3 14.0mag 78P/Gehrels
00:22:06.35 -01:13:55.0 15.1mag 88P/Howell
03:35:24.53 +27:05:40.1 15.1mag 93P/Lovas
05:53:20.68 +33:17:22.3 15.9mag 123P/West-Hartley
09:08:41.77 +25:28:00.7 16.3mag 124P/Mrkos
03:18:21.11 +17:16:27.1 16.4mag 128P/Shoemaker-Holt
03:43:57.77 +17:27:06.3 17.6mag 131P/Mueller
03:59:00.94 +19:23:58.5 11.7mag 141P/Machholz
04:02:50.79 +14:05:11.0 11.6mag 141P-A/Machholz
02:43:40.17 +10:28:08.1 10.5mag 141P-D/Machholz
02:39:17.34 -28:40:24.5 17.7mag 161P/Hartley-IRAS
02:23:57.50 +12:41:34.7 14.9mag 162P/SidingSpring
17:10:33.56 -10:31:02.2 16.2mag 235P/LINEAR
06:38:03.93 +35:53:54.8 17.2mag 240P/NEAT
07:56:38.16 -02:42:12.8 18.0mag 242P/Spahr
23:28:25.21 -12:09:21.9 17.1mag 260P/McNaught
03:00:56.80 +27:20:01.4 17.7mag 295P/LINEAR
15:28:18.87 +08:16:35.3 17.4mag 391P/Kowalski
07:49:06.96 +21:13:32.0 17.8mag 450P/LONEOS
06:19:42.70 +43:20:30.6 17.7mag 493P/LONEOS
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
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
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
12:59:50.45 -10:58:38.80 2026-05-9.06 17.5
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
12:59:50.45 -10:58:38.80 2026-05-9.06 17.5
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 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
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
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
-rw-r--r-- 1 apache apache 188K May 14 05:27 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:33:36.360 +46:45:22.36 AT 2026ltd 2026-05-07.31 19.8341
14:33:39.184 +62:53:16.81 AT 2026ltc 2026-05-07.24 20.2002
15:35:55.627 +08:44:12.14 AT 2026ltb 2026-05-08.44 19.483
14:06:38.410 +52:27:01.16 AT 2026lta 2026-05-07.24 19.8764
15:58:45.583 -26:43:14.65 AT 2026lsz 2026-05-08.42 19.9506
15:54:39.855 +46:28:35.62 AT 2026lsy 2026-05-07.31 19.8581
19:58:08.215 +01:50:57.83 AT 2026lsx 2026-05-09.41 19.7916
19:35:46.115 +01:05:02.22 AT 2026lsw 2026-05-08.40 19.7563
21:57:26.188 +07:29:34.54 AT 2026lsv 2026-05-09.48 19.7344
08:20:51.567 -28:13:50.92 AT 2026lsu 2026-05-08.26 18.852
00:17:43.918 +18:16:22.09 AT 2026lst 2026-05-07.49 18.3871
13:32:42.666 -34:54:34.19 AT 2026lss 2026-05-09.44 19.6
14:40:14.170 -19:17:59.48 AT 2026lsr 2026-05-09.47 19.94
14:25:36.624 -09:24:28.62 AT 2026lsq 2026-05-07.49 19.77
09:30:06.631 -13:35:53.35 AT 2026lsp 2026-05-05.36 19.93
10:56:02.293 -27:26:40.88 AT 2026lso 2026-05-05.38 20.03
13:09:18.098 -09:51:30.87 AT 2026lsn 2026-05-06.44 20.03
12:38:36.545 +00:25:39.42 AT 2026lsm 2026-05-07.49 20.12
14:09:44.920 -09:15:56.43 AT 2026lsl 2026-05-07.48 20.05
14:33:39.027 +28:55:58.13 AT 2026lsk 2026-05-08.42 18.836
-rw-r--r-- 1 apache apache 30K May 14 05:27 tns_transients_list.txt
