This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 12.11 01:40:59.96 +62:28:20.7
128.62328 0.14960 galactic Cas Second-epoch detections are separated by 2.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:40:59.96 +62:28:20.7 (user input) | T | P | (position from user input) J-Ks=0.588+/-0.040 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:59.96 +62:28:20.7: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:59.96 +62:28:20.7: 15.03 +/- 0.12 detection
Forced photometry reference-image weighted average: 15.03 +/- 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 07 07.4102* 01 40 59.96 +62 28 20.7 12.1 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,2461228.9102,12.11,0.05,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 20260707.4102 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 12.02 01:41:38.74 +63:03:45.9
128.58238 0.74313 galactic Cas Second-epoch detections are separated by 0.4" and 1.9 pix
The object was found in VSX14" Gaia DR3 511700758683269376
Type: ROT
# Max. Min./Amp. JD0 Period
16.450 G 16.500 G G
ATTENTION: measured mag 12.02 is 4.4 mag brighter than the VSX record maximum brightness 16.45 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:38.74 +63:03:45.9: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:38.74 +63:03:45.9: 14.63 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.63 +/- 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 07 07.4102* 01 41 38.74 +63 03 45.9 12.0 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 511700758683269376,2461228.9102,12.02,0.05,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 511700758683269376 20260707.4102 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.85 01:19:08.75 +60:17:19.5
126.36182 -2.39835 galactic Cas Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:19:08.75 +60:17:19.5 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.75 +60:17:19.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:08.75 +60:17:19.5: 14.72 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.72 +/- 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 07 07.4102* 01 19 08.75 +60 17 19.5 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
target,2461228.9102,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.85CV 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 07 07.4102 2461228.9102 11.63 01:34:23.30 +59:34:48.4
128.35167 -2.83891 galactic Cas Second-epoch detections are separated by 1.9" and 2.4 pix
The object was found in VSX19" Gaia DR3 509372061778119680
Type: ROT
# Max. Min./Amp. JD0 Period
14.510 G 14.540 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 01:34:23.30 +59:34:48.4: 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 01:34:23.30 +59:34:48.4: 14.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.39 +/- 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 07 07.4102* 01 34 23.30 +59 34 48.4 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 509372061778119680,2461228.9102,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509372061778119680 20260707.4102 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.69 01:52:15.83 +65:17:43.8
129.23528 3.17084 galactic Cas Second-epoch detections are separated by 2.2" and 1.8 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 | 01:52:15.83 +65:17:43.8 (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 01:52:15.83 +65:17:43.8: 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 01:52:15.83 +65:17:43.8: 14.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.11 +/- 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 07 07.4102* 01 52 15.83 +65 17 43.8 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.9102,11.69,0.05,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 20260707.4102 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.87 01:11:35.74 +60:37:33.4
125.40313 -2.14905 galactic Cas Second-epoch detections are separated by 2.3" and 1.8 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 | 01:11:35.74 +60:37:33.4 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:35.74 +60:37:33.4: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:35.74 +60:37:33.4: 14.36 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.36 +/- 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 07 07.4102* 01 11 35.74 +60 37 33.4 11.9 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,2461228.9102,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.63 01:06:15.75 +57:53:23.4
124.90823 -4.92502 galactic Cas Second-epoch detections are separated by 1.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J016.5720+57.8855 | 01:06:15.75 +57:53:23.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.781+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:15.75 +57:53:23.4: 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 01:06:15.75 +57:53:23.4: 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 07 07.4102* 01 06 15.75 +57 53 23.4 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
ATO J016.5720+57.8855,2461228.9102,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J016.5720+57.8855 20260707.4102 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.59 01:33:40.62 +59:42:24.0
128.24206 -2.72888 galactic Cas Second-epoch detections are separated by 1.9" and 2.0 pix
The object was found in VSX 0" ZTF J013340.67+594224.0
Type: SR
# Max. Min./Amp. JD0 Period
16.002 g Y 0.134 g 2458302.89690 31.071577300000
ATTENTION: measured mag 11.59 is 4.3 mag brighter than the VSX record maximum brightness 15.87 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:40.62 +59:42:24.0: 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 01:33:40.62 +59:42:24.0: 14.47 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.47 +/- 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 07 07.4102* 01 33 40.62 +59 42 24.0 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
ZTF J013340.67+594224.0,2461228.9102,11.59,0.05,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
ZTF J013340.67+594224.0 20260707.4102 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 07 07.4102 2461228.9102 11.43 01:33:12.67 +61:16:55.0
127.92959 -1.18380 galactic Cas Second-epoch detections are separated by 1.2" and 1.7 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 | 01:33:12.67 +61:16:55.0 (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 01:33:12.67 +61:16:55.0: 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 01:33:12.67 +61:16:55.0: 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 07 07.4102* 01 33 12.67 +61 16 55.0 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,2461228.9102,11.43,0.05,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 20260707.4102 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 07 07.4102 2461228.9102 11.50 01:57:29.16 +60:09:18.2
131.06667 -1.66938 galactic Cas Second-epoch detections are separated by 0.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:57:29.16 +60:09:18.2 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:29.16 +60:09:18.2: 12.99 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:29.16 +60:09:18.2: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 57 29.16 +60 09 18.2 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
target,2461228.9102,11.50,0.05,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 20260707.4102 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.46 01:10:32.20 +59:42:09.4
125.34209 -3.07973 galactic Cas Second-epoch detections are separated by 0.9" and 2.0 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 J017.6386+59.6997 | 01:10:32.20 +59:42:09.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.518+/-0.042 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:32.20 +59:42:09.4: 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 01:10:32.20 +59:42:09.4: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 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 07 07.4102* 01 10 32.20 +59 42 09.4 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
ATO J017.6386+59.6997,2461228.9102,11.46,0.05,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
ATO J017.6386+59.6997 20260707.4102 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 07 07.4102 2461228.9102 11.56 01:13:00.48 +62:45:32.3
125.39738 -0.00947 galactic Cas Second-epoch detections are separated by 1.4" and 1.6 pix
The object was found in VSX 2" Gaia DR3 523086613905448832
Type: ROT
# Max. Min./Amp. JD0 Period
14.430 G 14.470 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 01:13:00.48 +62:45:32.3: 12.83 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:00.48 +62:45:32.3: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 07 07.4102* 01 13 00.48 +62 45 32.3 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
Gaia DR3 523086613905448832,2461228.9102,11.56,0.05,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 523086613905448832 20260707.4102 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.69 01:23:01.77 +60:35:36.4
126.80294 -2.04064 galactic Cas Second-epoch detections are separated by 2.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:23:01.77 +60:35:36.4 (user input) | T | P | (position from user input) J-Ks=0.530+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:01.77 +60:35:36.4: 12.36 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:01.77 +60:35:36.4: 14.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 23 01.77 +60 35 36.4 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,2461228.9102,11.69,0.05,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 20260707.4102 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.38 01:09:00.43 +58:43:03.8
125.21680 -4.07606 galactic Cas Second-epoch detections are separated by 0.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 413764474854792192 | 01:09:00.43 +58:43:03.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.333+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:00.43 +58:43:03.8: 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 01:09:00.43 +58:43:03.8: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 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 07 07.4102* 01 09 00.43 +58 43 03.8 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
Large-amplitude variable Gaia DR2 413764474854792192,2461228.9102,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 413764474854792192 20260707.4102 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.38 01:17:42.54 +60:29:21.3
126.16417 -2.21752 galactic Cas Second-epoch detections are separated by 2.8" and 2.0 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 | 01:17:42.54 +60:29:21.3 (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 01:17:42.54 +60:29:21.3: 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 01:17:42.54 +60:29:21.3: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 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 07 07.4102* 01 17 42.54 +60 29 21.3 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.9102,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.60 01:31:56.02 +59:26:41.0
128.06588 -3.02276 galactic Cas Second-epoch detections are separated by 2.2" and 1.8 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 J023.0100+59.4551 | 01:31:59.23 +59:26:47.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1955ApJS....2..123F LF 5 +59 42 J-Ks=0.314+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:56.02 +59:26:41.0: 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 01:31:56.02 +59:26:41.0: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 07 07.4102* 01 31 56.02 +59 26 41.0 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
ATO J023.0100+59.4551,2461228.9102,11.60,0.05,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 J023.0100+59.4551 20260707.4102 11.60CV 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 07 07.4102 2461228.9102 11.40 01:07:01.76 +59:46:19.6
124.89589 -3.04017 galactic Cas Second-epoch detections are separated by 1.9" and 2.0 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 | 01:07:01.76 +59:46:19.6 (user input) | T | P | (position from user input) J-Ks=0.500+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:01.76 +59:46:19.6: 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 01:07:01.76 +59:46:19.6: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 07 01.76 +59 46 19.6 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,2461228.9102,11.40,0.05,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
target 20260707.4102 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 07 07.4102 2461228.9102 11.47 01:24:16.13 +59:08:33.2
127.13875 -3.46077 galactic Cas Second-epoch detections are separated by 3.0" and 2.5 pix
The object was found in VSX 3" Gaia DR3 510038675059657344
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.430 G 14.460 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 01:24:16.13 +59:08:33.2: 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 01:24:16.13 +59:08:33.2: 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 07 07.4102* 01 24 16.13 +59 08 33.2 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 510038675059657344,2461228.9102,11.47,0.05,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
Gaia DR3 510038675059657344 20260707.4102 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 07 07.4102 2461228.9102 11.27 01:12:41.14 +61:18:08.0
125.48067 -1.46433 galactic Cas Second-epoch detections are separated by 1.2" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:41.14 +61:18:08.0 (user input) | T | P | (position from user input) J-Ks=0.156+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:41.14 +61:18:08.0: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:41.14 +61:18:08.0: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 12 41.14 +61 18 08.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.9102,11.27,0.05,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 20260707.4102 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 07 07.4102 2461228.9102 11.38 01:10:07.90 +57:43:54.9
125.43472 -5.04896 galactic Cas Second-epoch detections are separated by 1.1" and 2.0 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 | 01:10:07.90 +57:43:54.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.731+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:07.90 +57:43:54.9: 11.82 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:07.90 +57:43:54.9: 14.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 07 07.4102* 01 10 07.90 +57 43 54.9 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,2461228.9102,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.19 01:32:22.89 +61:29:14.1
127.79870 -0.99701 galactic Cas Second-epoch detections are separated by 0.2" and 1.8 pix
The object was found in VSX13" Gaia DR3 510746485668934272
Type: ROT
# Max. Min./Amp. JD0 Period
15.470 G 15.520 G G
ATTENTION: measured mag 11.19 is 4.3 mag brighter than the VSX record maximum brightness 15.47 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:22.89 +61:29:14.1: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:22.89 +61:29:14.1: 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 07 07.4102* 01 32 22.89 +61 29 14.1 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
Gaia DR3 510746485668934272,2461228.9102,11.19,0.05,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
Gaia DR3 510746485668934272 20260707.4102 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 07 07.4102 2461228.9102 11.37 01:41:51.95 +60:08:22.4
129.17488 -2.11953 galactic Cas Second-epoch detections are separated by 0.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.4532+60.1341 | 01:41:51.95 +60:08:22.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.943+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:51.95 +60:08:22.4: 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 01:41:51.95 +60:08:22.4: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 07 07.4102* 01 41 51.95 +60 08 22.4 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
ATO J025.4532+60.1341,2461228.9102,11.37,0.05,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 20260707.4102 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.26 01:55:48.24 +58:53:45.3
131.17509 -2.94184 galactic Cas Second-epoch detections are separated by 1.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:55:48.24 +58:53:45.3 (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 01:55:48.24 +58:53:45.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:48.24 +58:53:45.3: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 07 07.4102* 01 55 48.24 +58 53 45.3 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
target,2461228.9102,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.25 01:26:16.97 +59:48:45.7
127.30464 -2.76289 galactic Cas Second-epoch detections are separated by 1.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:26:16.97 +59:48:45.7 (user input) | T | P | (position from user input) J-Ks=0.720+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:16.97 +59:48:45.7: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:16.97 +59:48:45.7: 13.77 +/- 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 07 07.4102* 01 26 16.97 +59 48 45.7 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
target,2461228.9102,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.20 01:41:44.33 +64:14:45.1
128.36335 1.90585 galactic Cas Second-epoch detections are separated by 3.7" and 1.6 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 512898161208515840 | 01:41:38.37 +64:14:54.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.140+/-0.051 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:44.33 +64:14:45.1: 12.01 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:44.33 +64:14:45.1: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 07 07.4102* 01 41 44.33 +64 14 45.1 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
Gaia DR3 512898161208515840,2461228.9102,11.20,0.05,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 512898161208515840 20260707.4102 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.27 01:12:15.26 +58:17:15.8
125.67311 -4.47319 galactic Cas Second-epoch detections are separated by 2.2" and 1.8 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 J018.0624+58.2786 | 01:12:15.26 +58:17:15.8 (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 01:12:15.26 +58:17:15.8: 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 01:12:15.26 +58:17:15.8: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 07 07.4102* 01 12 15.26 +58 17 15.8 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
ATO J018.0624+58.2786,2461228.9102,11.27,0.05,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
ATO J018.0624+58.2786 20260707.4102 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 07 07.4102 2461228.9102 11.17 01:56:12.92 +59:33:49.7
131.06050 -2.28174 galactic Cas Second-epoch detections are separated by 1.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:12.92 +59:33:49.7 (user input) | T | P | (position from user input) J-Ks=0.814+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:12.92 +59:33:49.7: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:12.92 +59:33:49.7: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 07 07.4102* 01 56 12.92 +59 33 49.7 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
target,2461228.9102,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.07 01:51:47.39 +58:37:55.4
130.73238 -3.32267 galactic Cas Second-epoch detections are separated by 2.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506225156418009984 | 01:51:45.68 +58:37:15.2 (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 01:51:47.39 +58:37:55.4: 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 01:51:47.39 +58:37:55.4: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 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 07 07.4102* 01 51 47.39 +58 37 55.4 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 506225156418009984,2461228.9102,11.07,0.05,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 20260707.4102 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 07 07.4102 2461228.9102 11.25 01:10:04.80 +57:48:02.7
125.42280 -4.98081 galactic Cas Second-epoch detections are separated by 3.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:10:04.80 +57:48:02.7 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:04.80 +57:48:02.7: 12.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:04.80 +57:48:02.7: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 07 07.4102* 01 10 04.80 +57 48 02.7 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
target,2461228.9102,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.10 01:28:32.62 +61:12:20.1
127.38630 -1.34484 galactic Cas Second-epoch detections are separated by 1.9" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | PQ Cas | 01:28:36.18 +61:12:07.5 (Gaia DR3) | SR (local) | 77.771904400000 (local) | Gaia3var=VARIABLE SpType: S 1975AbaOB..47....3D [D75b] Star 4 J-Ks=0.477+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:32.62 +61:12:20.1: 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 01:28:32.62 +61:12:20.1: 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 07 07.4102* 01 28 32.62 +61 12 20.1 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
PQ Cas,2461228.9102,11.10,0.05,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
PQ Cas 20260707.4102 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 07 07.4102 2461228.9102 11.10 01:15:23.10 +61:11:40.4
125.81358 -1.54314 galactic Cas Second-epoch detections are separated by 0.7" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510546374554030464 | 01:15:25.46 +61:11:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.305+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:23.10 +61:11:40.4: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:23.10 +61:11:40.4: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 15 23.10 +61 11 40.4 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 510546374554030464,2461228.9102,11.10,0.05,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 510546374554030464 20260707.4102 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 07 07.4102 2461228.9102 11.05 01:43:27.43 +58:38:05.3
129.67130 -3.55461 galactic Cas Second-epoch detections are separated by 0.0" and 2.3 pix
The object was found in VSX 0" Gaia DR3 506084487648397824
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:27.43 +58:38:05.3: 12.67 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.43 +58:38:05.3: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 43 27.43 +58 38 05.3 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 506084487648397824,2461228.9102,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506084487648397824 20260707.4102 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.01 01:12:59.73 +57:34:07.2
125.83101 -5.18168 galactic Cas Second-epoch detections are separated by 2.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:59.73 +57:34:07.2 (user input) | T | P | (position from user input) J-Ks=0.831+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:59.73 +57:34:07.2: 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 01:12:59.73 +57:34:07.2: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 12 59.73 +57 34 07.2 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,2461228.9102,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.07 01:11:58.85 +64:42:09.3
125.12533 1.91836 galactic Cas Second-epoch detections are separated by 2.0" and 1.1 pix
The object was found in VSX18" ZTF J011201.03+644221.2
Type: RS
# Max. Min./Amp. JD0 Period
14.762 g Y 0.263 g 2458343.85900 3.018403700000
ATTENTION: measured mag 11.07 is 3.4 mag brighter than the VSX record maximum brightness 14.50 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:58.85 +64:42:09.3: 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 01:11:58.85 +64:42:09.3: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 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 07 07.4102* 01 11 58.85 +64 42 09.3 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
ZTF J011201.03+644221.2,2461228.9102,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011201.03+644221.2 20260707.4102 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 07 07.4102 2461228.9102 11.08 01:09:10.40 +58:09:35.6
125.27697 -4.63108 galactic Cas Second-epoch detections are separated by 4.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:09:10.40 +58:09:35.6 (user input) | T | P | (position from user input) J-Ks=0.750+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:10.40 +58:09:35.6: 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 01:09:10.40 +58:09:35.6: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 09 10.40 +58 09 35.6 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,2461228.9102,11.08,0.05,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 20260707.4102 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 10.90 01:21:22.04 +60:51:44.8
126.56902 -1.79777 galactic Cas Second-epoch detections are separated by 0.6" and 1.8 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 510467759471265280 | 01:21:25.06 +60:51:43.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.619+/-0.045 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:22.04 +60:51:44.8: 11.22 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:22.04 +60:51:44.8: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.83 +/- 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 07 07.4102* 01 21 22.04 +60 51 44.8 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
Gaia DR3 510467759471265280,2461228.9102,10.90,0.05,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
Gaia DR3 510467759471265280 20260707.4102 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 07 07.4102 2461228.9102 10.97 01:07:31.92 +61:28:28.1
124.85265 -1.33724 galactic Cas Second-epoch detections are separated by 2.3" and 2.0 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 | 01:07:31.92 +61:28:28.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:31.92 +61:28:28.1: 12.92 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:31.92 +61:28:28.1: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 07 07.4102* 01 07 31.92 +61 28 28.1 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
target,2461228.9102,10.97,0.05,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 20260707.4102 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 07 07.4102 2461228.9102 10.68 01:31:23.04 +59:33:42.4
127.97866 -2.91798 galactic Cas Second-epoch detections are separated by 0.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J022.8294+59.5638 | 01:31:23.04 +59:33:42.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.833+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:23.04 +59:33:42.4: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:23.04 +59:33:42.4: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 07 07.4102* 01 31 23.04 +59 33 42.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.8294+59.5638,2461228.9102,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.8294+59.5638 20260707.4102 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 10.64 01:56:43.15 +58:07:17.5
131.48403 -3.66214 galactic Cas Second-epoch detections are separated by 1.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:43.15 +58:07:17.5 (user input) | T | P | (position from user input) J-Ks=0.952+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:43.15 +58:07:17.5: 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 01:56:43.15 +58:07:17.5: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 07 07.4102* 01 56 43.15 +58 07 17.5 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,2461228.9102,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 10.40 01:44:02.20 +61:52:11.0
129.08940 -0.37158 galactic Cas Second-epoch detections are separated by 0.3" and 2.0 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 511486353915154176 | 01:43:57.23 +61:52:41.4 (Gaia DR3) | VAR (local) | 0.018104900000 (local) | Gaia3var=NOT_AVAILABLE SpType: B3 1953IzKry..10..120K [K53] 513
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:02.20 +61:52:11.0: 12.07 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:02.20 +61:52:11.0: 14.22 +/- 0.29 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 44 02.20 +61 52 11.0 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
Gaia DR3 511486353915154176,2461228.9102,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511486353915154176 20260707.4102 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 10.71 01:52:47.75 +58:10:25.4
130.96819 -3.73744 galactic Cas Second-epoch detections are separated by 0.7" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J028.1896+58.1775 | 01:52:46.32 +58:10:45.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.086+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:47.75 +58:10:25.4: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:47.75 +58:10:25.4: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 52 47.75 +58 10 25.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J028.1896+58.1775,2461228.9102,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J028.1896+58.1775 20260707.4102 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 10.84 01:51:09.25 +64:52:45.2
129.21802 2.73881 galactic Cas Second-epoch detections are separated by 2.9" and 1.4 pix
The object was found in VSX 4" Gaia DR3 518229967963921664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:09.25 +64:52:45.2: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.25 +64:52:45.2: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 51 09.25 +64 52 45.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 518229967963921664,2461228.9102,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518229967963921664 20260707.4102 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 10.89 01:34:32.01 +60:30:13.0
128.21591 -1.92525 galactic Cas Second-epoch detections are separated by 1.3" and 1.9 pix
The object was found in VSX24" Gaia DR3 509857290009059456
Type: RS
# Max. Min./Amp. JD0 Period
17.420 G 17.560 G F
ATTENTION: measured mag 10.89 is 6.5 mag brighter than the VSX record maximum brightness 17.42 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:32.01 +60:30:13.0: 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 01:34:32.01 +60:30:13.0: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 07 07.4102* 01 34 32.01 +60 30 13.0 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 509857290009059456,2461228.9102,10.89,0.05,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
Gaia DR3 509857290009059456 20260707.4102 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 07 07.4102 2461228.9102 10.91 01:10:45.61 +64:05:35.1
125.04096 1.30049 galactic Cas Second-epoch detections are separated by 1.0" and 1.3 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 523447872192664448 | 01:10:43.44 +64:04:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1960IzKry..24..160B [B60] +63 52
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:45.61 +64:05:35.1: 11.14 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:45.61 +64:05:35.1: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 07 07.4102* 01 10 45.61 +64 05 35.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523447872192664448,2461228.9102,10.91,0.05,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
Gaia DR3 523447872192664448 20260707.4102 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 07 07.4102 2461228.9102 11.02 01:11:56.65 +58:41:05.1
125.60060 -4.08070 galactic Cas Second-epoch detections are separated by 1.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.9933+58.6776 | 01:11:56.65 +58:41:05.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.669+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:56.65 +58:41:05.1: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:56.65 +58:41:05.1: 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 07 07.4102* 01 11 56.65 +58 41 05.1 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 J017.9933+58.6776,2461228.9102,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.9933+58.6776 20260707.4102 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 10.95 02:15:50.61 +63:12:33.0
132.27586 1.87896 galactic Cas Second-epoch detections are separated by 1.6" and 1.8 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 | 02:15:50.61 +63:12:33.0 (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 02:15:50.61 +63:12:33.0: 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 02:15:50.61 +63:12:33.0: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 07 07.4102* 02 15 50.61 +63 12 33.0 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,2461228.9102,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.04 01:48:29.79 +60:27:33.3
129.91266 -1.63685 galactic Cas Second-epoch detections are separated by 0.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:48:29.79 +60:27:33.3 (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 01:48:29.79 +60:27:33.3: 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 01:48:29.79 +60:27:33.3: 13.79 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 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 07 07.4102* 01 48 29.79 +60 27 33.3 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
target,2461228.9102,11.04,0.05,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 20260707.4102 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 07 07.4102 2461228.9102 10.98 02:15:03.85 +58:28:53.1
133.69490 -2.63192 galactic Per Second-epoch detections are separated by 1.5" and 2.6 pix
The object was found in VSX 2" 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 02:15:03.85 +58:28:53.1: 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 02:15:03.85 +58:28:53.1: 13.72 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 07 07.4102* 02 15 03.85 +58 28 53.1 11.0 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 506806798067617152,2461228.9102,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506806798067617152 20260707.4102 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.17 01:23:53.48 +60:53:24.3
126.87068 -1.73323 galactic Cas Second-epoch detections are separated by 1.1" and 1.7 pix
The object was found in VSX25" Gaia DR3 510306577943067520
Type: E
# Max. Min./Amp. JD0 Period
17.750 G 18.070 G 2.951710000000
ATTENTION: measured mag 11.17 is 6.6 mag brighter than the VSX record maximum brightness 17.75 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:53.48 +60:53:24.3: 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 01:23:53.48 +60:53:24.3: 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 07 07.4102* 01 23 53.48 +60 53 24.3 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 510306577943067520,2461228.9102,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510306577943067520 20260707.4102 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.16 01:38:11.78 +65:33:01.0
127.74948 3.11683 galactic Cas Second-epoch detections are separated by 1.3" and 1.6 pix
The object was found in VSX 2" ASASSN-V J013812.08+653302.3
Type: L
# Max. Min./Amp. JD0 Period
14.260 V 14.420 V
ATTENTION: measured mag 11.16 is 3.1 mag brighter than the VSX record maximum brightness 14.26 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:11.78 +65:33:01.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:11.78 +65:33:01.0: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 07 07.4102* 01 38 11.78 +65 33 01.0 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
ASASSN-V J013812.08+653302.3,2461228.9102,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013812.08+653302.3 20260707.4102 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.16 01:08:59.23 +60:47:20.2
125.07277 -2.00984 galactic Cas Second-epoch detections are separated by 1.1" and 2.0 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 522440066710315904 | 01:08:58.80 +60:47:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.504+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:59.23 +60:47:20.2: 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 01:08:59.23 +60:47:20.2: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 08 59.23 +60 47 20.2 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
Gaia DR3 522440066710315904,2461228.9102,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522440066710315904 20260707.4102 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.20 01:10:04.88 +60:32:45.1
125.22362 -2.24290 galactic Cas Second-epoch detections are separated by 1.3" and 1.8 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 | Large-amplitude variable Gaia DR2 426345911537396096 | 01:10:02.14 +60:33:00.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F8 1935BSD...C01....0S BSD 8-1180 J-Ks=0.592+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:04.88 +60:32:45.1: 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 01:10:04.88 +60:32:45.1: 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 07 07.4102* 01 10 04.88 +60 32 45.1 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
Large-amplitude variable Gaia DR2 426345911537396096,2461228.9102,11.20,0.05,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
Large-amplitude variable Gaia DR2 426345911537396096 20260707.4102 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.05 01:14:41.46 +58:46:46.2
125.94854 -3.95598 galactic Cas Second-epoch detections are separated by 1.4" and 2.3 pix
The object was found in VSX23" Gaia DR3 414091266028390144
Type: ROT
# Max. Min./Amp. JD0 Period
18.000 G 18.140 G
ATTENTION: measured mag 11.05 is 6.9 mag brighter than the VSX record maximum brightness 18.00 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:41.46 +58:46:46.2: 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 01:14:41.46 +58:46:46.2: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 07 07.4102* 01 14 41.46 +58 46 46.2 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 414091266028390144,2461228.9102,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 414091266028390144 20260707.4102 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.20 01:15:11.19 +60:52:41.8
125.81890 -1.86028 galactic Cas Second-epoch detections are separated by 0.6" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:15:11.19 +60:52:41.8 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:11.19 +60:52:41.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:11.19 +60:52:41.8: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 07 07.4102* 01 15 11.19 +60 52 41.8 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,2461228.9102,11.20,0.05,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
target 20260707.4102 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.18 01:10:08.44 +62:43:49.5
125.07234 -0.06358 galactic Cas Second-epoch detections are separated by 1.6" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:10:08.44 +62:43:49.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:08.44 +62:43:49.5: 11.50 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:08.44 +62:43:49.5: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 07 07.4102* 01 10 08.44 +62 43 49.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.9102,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 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 07 07.4102 2461228.9102 11.22 01:34:07.12 +60:12:53.2
128.21318 -2.21859 galactic Cas Second-epoch detections are separated by 1.7" and 1.8 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 509777472336200448 | 01:34:01.93 +60:13:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0IV/V 1928MeUpp..37....1S BD+59 277 J-Ks=0.892+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:07.12 +60:12:53.2: 11.69 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:07.12 +60:12:53.2: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 07 07.4102* 01 34 07.12 +60 12 53.2 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
Gaia DR3 509777472336200448,2461228.9102,11.22,0.05,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 509777472336200448 20260707.4102 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 07 07.4102 2461228.9102 11.14 01:09:22.71 +57:26:30.7
125.35441 -5.34548 galactic Cas Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.3204+57.4562 | 01:09:17.29 +57:26:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.782+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.71 +57:26:30.7: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.71 +57:26:30.7: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 09 22.71 +57 26 30.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.3204+57.4562,2461228.9102,11.14,0.05,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 J017.3204+57.4562 20260707.4102 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 07 07.4102 2461228.9102 11.18 01:21:22.27 +59:45:49.9
126.69704 -2.88888 galactic Cas Second-epoch detections are separated by 4.6" and 1.4 pix
The object was found in VSX 2" ZTF J012122.56+594550.4
Type: SR
# Max. Min./Amp. JD0 Period
16.259 g Y 0.740 g 2458401.83190 315.216865100000 C
ATTENTION: measured mag 11.18 is 4.3 mag brighter than the VSX record maximum brightness 15.52 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:22.27 +59:45:49.9: 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 01:21:22.27 +59:45:49.9: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.25 +/- 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 07 07.4102* 01 21 22.27 +59 45 49.9 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
ZTF J012122.56+594550.4,2461228.9102,11.18,0.05,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 J012122.56+594550.4 20260707.4102 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 07 07.4102 2461228.9102 11.20 01:08:36.84 +60:44:54.0
125.03003 -2.05342 galactic Cas Second-epoch detections are separated by 0.9" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426363744241527552 | 01:08:34.66 +60:44:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8: 1935BSD...C01....0S BSD 8-1144 J-Ks=0.451+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:36.84 +60:44:54.0: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:36.84 +60:44:54.0: 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 07 07.4102* 01 08 36.84 +60 44 54.0 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 426363744241527552,2461228.9102,11.20,0.05,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 426363744241527552 20260707.4102 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.33 01:50:58.50 +58:51:12.5
130.57825 -3.13158 galactic Cas Second-epoch detections are separated by 1.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506419666894284800 | 01:51:01.58 +58:50:41.4 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: F2 1960IzKry..24..160B [B60] +58 514 J-Ks=0.353+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:58.50 +58:51:12.5: 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 01:50:58.50 +58:51:12.5: 14.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.33 +/- 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 07 07.4102* 01 50 58.50 +58 51 12.5 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 506419666894284800,2461228.9102,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506419666894284800 20260707.4102 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.29 01:59:34.10 +58:19:16.5
131.79614 -3.37309 galactic Cas Second-epoch detections are separated by 2.2" and 2.7 pix
The object was found in VSX 3" ASASSN-V J015934.40+581915.4
Type: SR
# Max. Min./Amp. JD0 Period
14.300 V 14.390 V 2457236.00000 444.000000000000
ATTENTION: measured mag 11.29 is 3.0 mag brighter than the VSX record maximum brightness 14.30 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:34.10 +58:19:16.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:34.10 +58:19:16.5: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.13 +/- 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 07 07.4102* 01 59 34.10 +58 19 16.5 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 J015934.40+581915.4,2461228.9102,11.29,0.05,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 J015934.40+581915.4 20260707.4102 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 07 07.4102 2461228.9102 11.07 01:17:30.55 +57:44:30.7
126.41836 -4.95329 galactic Cas Second-epoch detections are separated by 1.5" and 2.0 pix
The object was found in VSX24" Gaia DR3 413462384041502080
Type: ROT
# Max. Min./Amp. JD0 Period
16.660 G 16.730 G 1.024490000000 M
ATTENTION: measured mag 11.07 is 5.6 mag brighter than the VSX record maximum brightness 16.66 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:30.55 +57:44:30.7: 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 01:17:30.55 +57:44:30.7: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 17 30.55 +57 44 30.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413462384041502080,2461228.9102,11.07,0.05,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 413462384041502080 20260707.4102 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 07 07.4102 2461228.9102 11.30 01:19:29.26 +59:25:22.0
126.49829 -3.25460 galactic Cas Second-epoch detections are separated by 0.8" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 414042479505165696 | 01:19:30.78 +59:24:54.8 (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: G3 1935BSD...C01....0S BSD 8- 264 J-Ks=0.435+/-0.045 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:29.26 +59:25:22.0: 13.10 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:29.26 +59:25:22.0: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 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 07 07.4102* 01 19 29.26 +59 25 22.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 414042479505165696,2461228.9102,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 414042479505165696 20260707.4102 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.32 01:33:30.54 +58:02:22.4
128.49303 -4.37721 galactic Cas Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J023.3712+58.0394 | 01:33:30.54 +58:02:22.4 (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 01:33:30.54 +58:02:22.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:30.54 +58:02:22.4: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 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 07 07.4102* 01 33 30.54 +58 02 22.4 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.3712+58.0394,2461228.9102,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J023.3712+58.0394 20260707.4102 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.24 01:59:33.87 +63:37:08.5
130.41345 1.74123 galactic Cas Second-epoch detections are separated by 3.7" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:33.87 +63:37:08.5 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:33.87 +63:37:08.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:33.87 +63:37:08.5: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 59 33.87 +63 37 08.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.9102,11.24,0.05,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 20260707.4102 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 07 07.4102 2461228.9102 11.34 01:29:25.33 +60:01:31.5
127.66448 -2.49684 galactic Cas Second-epoch detections are separated by 3.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:25.33 +60:01:31.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:25.33 +60:01:31.5: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:25.33 +60:01:31.5: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 07 07.4102* 01 29 25.33 +60 01 31.5 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,2461228.9102,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.26 01:24:35.75 +59:32:42.7
127.12858 -3.05610 galactic Cas Second-epoch detections are separated by 3.6" and 2.5 pix
The object was found in VSX19" Gaia DR3 510086538176193664
Type: ROT
# Max. Min./Amp. JD0 Period
15.760 G 15.790 G 5.255500000000 G
ATTENTION: measured mag 11.26 is 4.5 mag brighter than the VSX record maximum brightness 15.76 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:35.75 +59:32:42.7: 12.81 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:35.75 +59:32:42.7: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.99 +/- 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 07 07.4102* 01 24 35.75 +59 32 42.7 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 510086538176193664,2461228.9102,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510086538176193664 20260707.4102 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.27 01:41:34.38 +59:13:57.5
129.31461 -3.01640 galactic Cas Second-epoch detections are separated by 2.4" and 1.8 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 | 01:41:34.38 +59:13:57.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:34.38 +59:13:57.5: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:34.38 +59:13:57.5: 14.08 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.08 +/- 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 07 07.4102* 01 41 34.38 +59 13 57.5 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,2461228.9102,11.27,0.05,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 20260707.4102 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 07 07.4102 2461228.9102 11.38 01:54:05.81 +61:05:12.0
130.43387 -0.86912 galactic Cas Second-epoch detections are separated by 2.0" and 1.8 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 | 01:54:05.81 +61:05:12.0 (user input) | T | P | (position from user input) J-Ks=1.062+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:05.81 +61:05:12.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:05.81 +61:05:12.0: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 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 07 07.4102* 01 54 05.81 +61 05 12.0 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,2461228.9102,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.38 01:13:18.84 +63:56:03.8
125.33256 1.16465 galactic Cas Second-epoch detections are separated by 2.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:13:18.84 +63:56:03.8 (user input) | T | P | (position from user input) J-Ks=0.838+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:18.84 +63:56:03.8: 11.58 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:18.84 +63:56:03.8: 14.46 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 07 07.4102* 01 13 18.84 +63 56 03.8 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
target,2461228.9102,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.22 02:02:25.13 +64:38:23.5
130.44187 2.80810 galactic Cas Second-epoch detections are separated by 7.1" and 1.0 pix
The object was found in VSX 5" 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 02:02:25.13 +64:38:23.5: 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 02:02:25.13 +64:38:23.5: 14.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 07 07.4102* 02 02 25.13 +64 38 23.5 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
ASASSN-V J020225.96+643822.9,2461228.9102,11.22,0.05,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
ASASSN-V J020225.96+643822.9 20260707.4102 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 07 07.4102 2461228.9102 11.32 01:19:08.10 +60:33:39.2
126.33124 -2.12792 galactic Cas Second-epoch detections are separated by 0.7" and 1.8 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 510378080556092032 | 01:19:06.00 +60:34:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.495+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.10 +60:33:39.2: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:08.10 +60:33:39.2: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.4102* 01 19 08.10 +60 33 39.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510378080556092032,2461228.9102,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510378080556092032 20260707.4102 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.59 01:54:07.38 +61:05:02.3
130.43759 -0.87098 galactic Cas Second-epoch detections are separated by 1.9" and 1.8 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 | 01:54:07.38 +61:05:02.3 (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 01:54:07.38 +61:05:02.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:07.38 +61:05:02.3: 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 07 07.4102* 01 54 07.38 +61 05 02.3 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,2461228.9102,11.59,0.05,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
target 20260707.4102 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 07 07.4102 2461228.9102 11.55 01:20:06.59 +60:14:18.5
126.48625 -2.43526 galactic Cas Second-epoch detections are separated by 3.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:20:06.59 +60:14:18.5 (user input) | T | P | (position from user input) J-Ks=1.078+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:06.59 +60:14:18.5: 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 01:20:06.59 +60:14:18.5: 14.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.25 +/- 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 07 07.4102* 01 20 06.59 +60 14 18.5 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,2461228.9102,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.4102 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.44 02:01:06.28 +64:35:47.0
130.31779 2.72833 galactic Cas Second-epoch detections are separated by 6.5" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 518077479449762560 | 02:01:07.64 +64:35:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:06.28 +64:35:47.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:06.28 +64:35:47.0: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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 07 07.4102* 02 01 06.28 +64 35 47.0 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 518077479449762560,2461228.9102,11.44,0.05,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
Gaia DR3 518077479449762560 20260707.4102 11.44CV 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 07 07.4102 2461228.9102 11.52 01:38:35.70 +64:48:51.2
127.92426 2.40055 galactic Cas Second-epoch detections are separated by 2.0" and 1.6 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 513065252614504576 | 01:38:36.54 +64:48:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.864+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:35.70 +64:48:51.2: 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 01:38:35.70 +64:48:51.2: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 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 07 07.4102* 01 38 35.70 +64 48 51.2 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 513065252614504576,2461228.9102,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 513065252614504576 20260707.4102 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.63 01:48:17.77 +60:40:23.1
129.84179 -1.43359 galactic Cas Second-epoch detections are separated by 2.3" and 2.0 pix
The object was found in VSX10" Gaia DR3 511167701701981184
Type: ROT
# Max. Min./Amp. JD0 Period
17.690 G 17.800 G 10.278600000000
ATTENTION: measured mag 11.63 is 6.1 mag brighter than the VSX record maximum brightness 17.69 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:17.77 +60:40:23.1: 13.00 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:17.77 +60:40:23.1: 14.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.20 +/- 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 07 07.4102* 01 48 17.77 +60 40 23.1 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 511167701701981184,2461228.9102,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511167701701981184 20260707.4102 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.66 01:43:17.73 +60:46:50.7
129.22131 -1.45618 galactic Cas Second-epoch detections are separated by 2.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509729609217329536 | 01:43:12.00 +60:47:00.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 1955ApJS....2..123F LF 5 +60 205 J-Ks=0.443+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:17.73 +60:46:50.7: 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 01:43:17.73 +60:46:50.7: 14.43 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.43 +/- 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 07 07.4102* 01 43 17.73 +60 46 50.7 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 509729609217329536,2461228.9102,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509729609217329536 20260707.4102 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.62 01:32:37.51 +59:38:48.6
128.12054 -2.80934 galactic Cas Second-epoch detections are separated by 1.7" and 2.0 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 509387248782084480 | 01:32:32.61 +59:38:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1955ApJS....2..123F LF 5 +59 45 J-Ks=0.968+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:37.51 +59:38:48.6: 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 01:32:37.51 +59:38:48.6: 14.38 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.38 +/- 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 07 07.4102* 01 32 37.51 +59 38 48.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509387248782084480,2461228.9102,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509387248782084480 20260707.4102 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.4102 2461228.9102 11.88 01:08:30.34 +61:29:21.9
124.96770 -1.31485 galactic Cas Second-epoch detections are separated by 1.4" and 2.0 pix
The object was found in VSX 6" Gaia DR3 522530497240884736
Type: ROT
# Max. Min./Amp. JD0 Period
18.410 G 18.550 G
ATTENTION: measured mag 11.88 is 6.5 mag brighter than the VSX record maximum brightness 18.41 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:30.34 +61:29:21.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:30.34 +61:29:21.9: 14.80 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.80 +/- 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 07 07.4102* 01 08 30.34 +61 29 21.9 11.9 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 522530497240884736,2461228.9102,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522530497240884736 20260707.4102 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.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_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461228.90990256
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_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits'
wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.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_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:57.331 +62:00:38.42 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 01:42:57.331 +62:00:38.42
Angular distance between the image centers 0.0615 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:55.906 +62:00:33.36 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 01:42:55.906 +62:00:33.36
Angular distance between the image centers 0.0584 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 01:42:57.331 +62:00:38.42
Second-epoch second image center 01:42:55.906 +62:00:33.36
Angular distance between the image centers 0.00312 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.LjB7Lc8Mn4
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.VzzAxlsKya
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_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits &> /tmp/tmp.oFuFidnz7Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits &> /tmp/tmp.qiL2ssnlTQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.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.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-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.wcscat
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.wcscat
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.wcscat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat' -> '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.
ERROR: only 24 of 31559 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.08%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929150
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: 10000)
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
2.4 pix fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.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_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
14.6 mag. fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.LjB7Lc8Mn4 (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_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/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.wcscat 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.wcscat 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.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, bad_region=8115, passed=31559
Got 31559 stars (including 20507 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
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 272 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 181 matched stars entering correct_measured_positions(), 127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 166 matched stars entering correct_measured_positions(), 5658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.17"
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 329 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 253 matched stars entering correct_measured_positions(), 5719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.16"
Accuracy estimation diagnostic: 250 matched stars entering correct_measured_positions(), 8204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.77"
Excluding outliers - 250 stars left (next iteration limit 182)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=250 sigma_overall_arcsec=18.752 sigma_q1_arcsec=37.068 sigma_q2_arcsec=15.069 sigma_q3_arcsec=23.291 sigma_q4_arcsec=16.683 n_q1=21 n_q2=98 n_q3=46 n_q4=85 worst_quadrant_to_overall_ratio=1.977
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.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.wcscat.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.wcscat.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.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VzzAxlsKya (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_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/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.wcscat 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.wcscat 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.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, bad_region=8179, passed=31681
Got 31681 stars (including 20613 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat
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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 975 stars left (next iteration limit 1072)
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=975 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.289 n_q1=173 n_q2=179 n_q3=388 n_q4=235 worst_quadrant_to_overall_ratio=1.235
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.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.wcscat.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.wcscat.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.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.oFuFidnz7Y (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.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_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1566, bad_region=3913, passed=18975
Got 18975 stars (including 13822 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits.wcscat
util/solve_plate_with_UCAC5 got 18975 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 15539 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 15541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 15540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits N_match=969 sigma_overall_arcsec=0.523 sigma_q1_arcsec=0.509 sigma_q2_arcsec=0.487 sigma_q3_arcsec=0.577 sigma_q4_arcsec=0.541 n_q1=320 n_q2=299 n_q3=226 n_q4=124 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits -region wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qiL2ssnlTQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.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_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1596, bad_region=3926, passed=18905
Got 18905 stars (including 13738 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits.wcscat
util/solve_plate_with_UCAC5 got 18905 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 15414 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 15416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 15416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits N_match=971 sigma_overall_arcsec=0.529 sigma_q1_arcsec=0.499 sigma_q2_arcsec=0.507 sigma_q3_arcsec=0.549 sigma_q4_arcsec=0.525 n_q1=325 n_q2=293 n_q3=232 n_q4=121 worst_quadrant_to_overall_ratio=1.039
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits -region wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=18.752 worst_q_ratio=1.977
ref2=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.376 worst_q_ratio=1.235
new1=fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits sigma_overall=0.523 worst_q_ratio=1.105
new2=fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits sigma_overall=0.529 worst_q_ratio=1.039
reference average sigma_overall=9.564 worst_q_ratio=1.606
warn-on-ratio threshold: 2.0x reference
###################################
ERROR: reference image Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a bad plate solution (astrometric residuals 18.752 arcsec while the other reference image of the same field has 0.376 arcsec) - the magnitude calibration relying on it is unreliable
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (250 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 8.01 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (975 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442_astrometric_residuals.png (969 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443_astrometric_residuals.png (971 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-05_20.00sec_4.90C_LIGHT_0442.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q2b1x1_050517_TTUQ2b1x1_3966691_atoHzQbx/wcs_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443.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 01:20:18.25 +64:28:04.2: 12.69 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:18.25 +64:28:04.2: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter REJECTED candidate at 01:20:18.25 +64:28:04.2: ref_mag=12.57 +/- 0.01 new_mean_mag=11.8294 delta=0.74 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 52511_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 52511_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:19:46.46 +58:12:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54953_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 54953_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
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Considering the candidate 20109_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 20109_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:56:37.96 +59:15:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 08339_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:20:32.36 +62:32:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29658_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 29658_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:09:23.45 +61:36:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247692_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247692_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247694_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247694_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247695_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247695_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:15:32.35 +60:23:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247696_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247696_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247703_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247703_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247706_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247706_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247707_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247707_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247709_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247709_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247714_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247714_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:10:12.09 +59:17:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247715_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247715_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247724_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247724_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247730_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247730_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247732_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247732_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:09:24.40 +58:01:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247734_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247734_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247737_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247737_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247739_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247739_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247744_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247744_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:47:52.81 +61:11:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247745_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247745_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:30:06.76 +61:51:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247747_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247747_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247751_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247751_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247754_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247754_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247756_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247756_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:13:39.09 +63:12:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247761_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247761_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:14:39.40 +59:25:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247764_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247764_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247765_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247765_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:39:59.12 +60:24:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247767_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247767_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247771_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247771_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247772_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247772_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247773_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247773_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:29:02.71 +58:46:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247776_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247776_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 247777_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247777_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247779_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247779_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:13:40.88 +60:51:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247781_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247781_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247783_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247783_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:08:25.55 +59:48:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247788_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247788_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:43:07.90 +58:54:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247789_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247789_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
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Considering the candidate 247790_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247790_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247793_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247793_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:33:01.43 +59:16:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247794_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247794_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247798_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247798_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:07:34.89 +57:33:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247805_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247805_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247806_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247806_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:07:39.02 +59:59:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247808_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247808_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:25:45.60 +59:01:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247811_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247811_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
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Considering the candidate 247813_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247813_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247816_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247816_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:26:36.73 +59:41:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247817_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247817_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247821_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247821_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:39:24.00 +58:23:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247824_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247824_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:58:54.76 +58:10:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247828_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247828_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247830_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247830_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:08:23.27 +61:35:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247831_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 247831_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 247838_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247838_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:01:30.55 +65:05:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247841_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247841_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:30:10.12 +59:36:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247845_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247845_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:09:29.75 +61:47:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247846_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247846_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:32:21.98 +60:27:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247852_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247852_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:05:57.37 +63:03:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247853_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247853_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:14:45.15 +60:30:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247854_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247854_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:07:57.20 +63:37:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247857_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247857_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:07:07.97 +57:44:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247858_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247858_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:25:26.43 +60:57:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247861_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247861_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:12:40.95 +61:20:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247862_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247862_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:35:24.78 +60:39:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247863_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247863_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:43:59.15 +61:55:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247866_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247866_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:55:14.46 +59:32:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247867_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247867_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:16:20.73 +62:42:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247869_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247869_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:15:30.60 +63:53:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247872_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247872_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:51:35.70 +57:52:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247873_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 247873_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:22:08.31 +60:22:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248739_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 248739_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 249020_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 249020_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 249087_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 249087_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 251609_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 251609_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:19:11.04 +58:20:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251651_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 251651_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:44:02.02 +61:53:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251818_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 251818_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:46:08.57 +61:12:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252053_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 252053_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:38:00.45 +57:56:45.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252200_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 252200_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 253198_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 253198_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:17:59.15 +57:47:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253387_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 253387_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:12:06.09 +59:41:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253503_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 253503_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:08:15.74 +63:34:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253535_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 253535_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:40:01.28 +60:52:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254237_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 254237_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:26:46.65 +57:46:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254367_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 254367_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:25:42.86 +65:40:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254824_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 254824_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:58:16.23 +59:38:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255588_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 255588_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 255703_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 255703_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:05:03.61 +64:21:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255779_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 255779_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:18:14.10 +61:44:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255873_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 255873_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
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Considering the candidate 255987_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 255987_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 256386_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 256386_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 256420_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 256420_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:26:41.19 +60:46:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256481_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 256481_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:20:10.93 +58:12:08.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256819_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 256819_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:46:33.55 +61:16:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256921_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 256921_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:16:08.65 +58:49:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256970_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 256970_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:18:19.10 +57:42:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257013_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 257013_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:44:17.61 +61:53:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257179_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 257179_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:43:53.11 +61:53:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257267_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 257267_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 257564_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 257564_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 257712_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 257712_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:20:18.44 +58:13:42.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 257728_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 257728_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:51:02.73 +64:49:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257763_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 257763_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:25:50.28 +61:06:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258124_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 258124_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258416_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 258416_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:44:32.29 +58:45:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258492_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 258492_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:02:54.81 +64:24:59.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 258585_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 258585_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:10:34.53 +60:31:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258889_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 258889_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:15:58.67 +63:12:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259075_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 259075_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:00:36.75 +58:30:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259240_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 259240_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 259317_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 259317_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:13:30.30 +58:34:24.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259745_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 259745_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:27:52.69 +62:46:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259793_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 259793_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:07:40.67 +63:30:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259909_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 259909_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:33:32.54 +60:40:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260230_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260230_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:13:35.94 +57:52:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260294_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260294_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:06:45.34 +59:50:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260433_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260433_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:19:22.27 +58:19:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260623_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260623_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:04:26.63 +65:05:51.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 260648_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260648_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:35:50.50 +61:27:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260684_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260684_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:19:03.81 +63:57:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260719_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260719_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:15:11.52 +60:07:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260727_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260727_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:37:44.72 +64:45:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260766_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260766_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:39:56.71 +60:52:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260893_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260893_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:10:31.42 +60:31:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260980_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 260980_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:20:13.94 +65:31:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261055_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 261055_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:16:05.16 +58:49:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261274_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 261274_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:58:04.11 +57:58:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261456_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 261456_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:43:06.91 +58:57:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261538_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 261538_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:42:33.09 +63:52:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261662_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 261662_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:10:23.73 +60:01:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261792_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 261792_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:24:45.28 +63:08:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261831_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 261831_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:18:36.80 +58:41:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261853_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 261853_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:08:30.53 +58:24:17.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261917_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 261917_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:27:02.28 +58:03:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262109_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262109_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:01:36.71 +59:57:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262195_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262195_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:34:10.27 +62:09:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262258_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262258_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:35:54.26 +60:13:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262396_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262396_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:19:41.72 +62:51:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262527_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262527_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:06:23.48 +62:44:01.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262536_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262536_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:15:52.80 +62:15:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262578_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262578_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:16:12.64 +62:42:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262583_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262583_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:47:19.07 +63:38:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262677_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262677_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:38:33.66 +60:47:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262687_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262687_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:44:56.47 +59:46:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262712_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262712_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:00:21.61 +64:56:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262792_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262792_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:49:34.30 +61:03:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262887_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 262887_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:22:23.83 +61:13:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263054_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 263054_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 263365_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 263365_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:02:53.82 +60:15:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263409_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 263409_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:46:38.44 +60:07:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263652_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 263652_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:08:33.12 +63:34:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263823_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 263823_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:07:24.53 +60:56:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263839_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 263839_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 263936_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 263936_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:03:15.22 +62:12:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263989_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 263989_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 264028_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264028_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:11:35.48 +57:37:25.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 264069_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264069_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
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Considering the candidate 264109_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 264109_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 264177_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264177_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:01:38.84 +61:45:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264231_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264231_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:18:48.30 +64:12:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264262_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264262_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
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Considering the candidate 264271_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264271_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:29:17.79 +62:38:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264305_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264305_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:36:16.43 +60:12:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264386_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264386_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:56:32.21 +59:56:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264447_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264447_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:37:13.31 +58:38:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264468_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264468_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:23:07.50 +61:11:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264474_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264474_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:54:34.77 +59:52:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264508_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264508_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:01:15.01 +59:23:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264534_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264534_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:55:52.73 +64:15:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264596_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264596_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:14:00.32 +61:42:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264730_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264730_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:14:00.60 +59:02:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264877_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264877_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:43:12.74 +64:00:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264936_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264936_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:22:58.25 +59:48:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264978_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 264978_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265036_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 265036_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265159_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265159_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:42:28.33 +58:17:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265185_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265185_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:29:32.82 +63:19:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265208_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265208_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:37:12.98 +58:38:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265236_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265236_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:07:03.83 +59:18:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265343_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265343_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:38:11.94 +61:01:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265465_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265465_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:31:29.14 +58:12:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265516_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 265516_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265550_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265550_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:21:28.94 +63:55:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265619_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265619_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:31:32.46 +61:02:19.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265708_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265708_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:26:05.49 +59:01:14.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265717_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265717_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:42:54.82 +64:01:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265731_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265731_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:20:49.29 +64:40:20.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265792_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265792_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:46:50.76 +60:39:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265883_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265883_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:42:26.68 +59:34:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265956_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265956_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:38:07.59 +61:01:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265963_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265963_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:28:07.36 +59:53:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265996_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 265996_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:54:30.31 +59:06:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266059_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 266059_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266119_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266119_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:43:03.27 +58:57:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266127_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266127_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:48:39.90 +59:09:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266157_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266157_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:58:04.75 +59:36:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266480_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266480_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:46:18.18 +60:59:19.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266555_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266555_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:32:40.35 +61:07:37.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266565_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 266565_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266652_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266652_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:29:21.43 +61:44:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266663_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266663_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:33:24.79 +58:21:30.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266741_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266741_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:37:41.48 +58:37:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266743_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266743_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:15:06.81 +60:09:20.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266745_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266745_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:34:42.52 +58:42:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266796_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 266796_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266976_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266976_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:52:55.02 +59:33:30.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266992_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 266992_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:14:21.78 +59:59:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267000_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267000_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:18:04.22 +65:36:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267224_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267224_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:37:55.28 +58:08:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267456_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267456_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:19:12.10 +65:35:57.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267505_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267505_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:16:36.67 +64:56:40.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267531_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267531_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:59:05.87 +59:55:34.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267534_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267534_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:34:34.30 +65:48:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267565_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267565_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:06:55.28 +59:18:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267661_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267661_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:20:40.59 +60:23:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267755_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267755_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:41:54.45 +62:34:05.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267870_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 267870_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267880_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 267880_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:27:03.88 +64:43:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268088_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268088_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:05:51.59 +60:27:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268132_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 268132_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268168_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268168_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:00:32.70 +59:40:07.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268258_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268258_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:56:25.39 +62:05:28.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268284_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 268284_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268295_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 268295_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268316_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268316_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:23:17.23 +58:25:14.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268322_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 268322_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268330_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268330_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:33:46.82 +62:31:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268331_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268331_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:38:05.70 +61:04:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268396_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268396_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:27:56.41 +62:46:06.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268569_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268569_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:36:13.61 +60:48:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268585_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268585_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:41:13.68 +62:53:20.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268654_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268654_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:44:32.25 +61:36:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268659_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268659_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:20:50.42 +58:20:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268705_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 268705_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 268727_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268727_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:01:03.44 +64:43:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268767_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268767_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:31:48.35 +64:21:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268785_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268785_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:38:06.53 +58:10:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268919_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268919_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:15:05.47 +64:08:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268924_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268924_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:19:28.76 +59:54:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268925_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 268925_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 268943_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 268943_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 268945_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 268945_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:29:49.61 +58:44:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268998_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 268998_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269174_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 269174_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:38:57.07 +63:28:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269259_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 269259_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:50:39.71 +62:00:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269352_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 269352_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:55:05.07 +59:57:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269386_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 269386_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 269398_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 269398_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:17:01.53 +63:21:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269495_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 269495_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:11:49.82 +59:02:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269611_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 269611_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:31:48.51 +64:22:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270029_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 270029_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:49:06.31 +65:23:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270113_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 270113_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:41:41.09 +57:56:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270146_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 270146_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:21:23.64 +63:43:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270171_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 270171_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 270297_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 270297_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:14:17.01 +60:56:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270321_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 270321_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 270470_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 270470_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 270491_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 270491_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 270668_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 270668_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 270762_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 270762_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 270862_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 270862_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:17:48.50 +58:35:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270922_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 270922_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
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Considering the candidate 270950_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 270950_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:07:28.97 +63:11:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270954_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 270954_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 271049_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 271049_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:48:34.85 +58:41:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271179_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 271179_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:40:47.06 +65:05:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271324_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 271324_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:36:31.71 +64:27:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271332_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 271332_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:16:55.73 +62:27:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271477_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 271477_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 271490_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 271490_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 272118_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 272118_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 272207_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 272207_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:46:23.86 +59:12:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272226_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 272226_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 272628_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 272628_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 272873_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 272873_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 272889_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 272889_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:44:29.86 +65:09:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272918_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 272918_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 272921_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 272921_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:23:24.72 +58:10:16.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272974_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 272974_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
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Considering the candidate 273283_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 273283_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 273813_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 273813_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 273839_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 273839_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:32:54.29 +60:17:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 274246_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 274246_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:24:45.12 +60:36:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 274280_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 274280_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 274722_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 274722_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 274795_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 274795_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 275342_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 275342_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 275488_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 275488_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:17:40.45 +58:13:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 275863_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 275863_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 275897_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 275897_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 276541_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 276541_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 279601_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
Preparing report for the candidate 279601_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
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Considering the candidate 196494_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 196494_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:01:27.95 +58:18:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173490_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 173490_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:22:51.66 +57:50:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 112593_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:21:55.07 +61:20:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 72532_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:45:35.71 +63:07:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186036_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 186036_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:38:43.78 +58:15:46.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 70271_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:20:32.30 +62:32:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156692_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 156692_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:56:37.99 +59:15:34.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 76113_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 02:02:02.24 +62:41:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 39378_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
**** FOUND 01:47:55.60 +64:32:54.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184075_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443
The candidate 184075_fd_Cas-03-Q2b1x1_2026-07-07_04-50-54_20.00sec_4.90C_LIGHT_0443 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 219s
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 ####
01:40:59.96 +62:28:20.7
01:41:38.74 +63:03:45.9
01:19:08.75 +60:17:19.5
01:34:23.30 +59:34:48.4
01:52:15.83 +65:17:43.8
01:11:35.74 +60:37:33.4
01:06:15.75 +57:53:23.4
01:33:40.62 +59:42:24.0
01:33:12.67 +61:16:55.0
01:57:29.16 +60:09:18.2
01:10:32.20 +59:42:09.4
01:13:00.48 +62:45:32.3
01:23:01.77 +60:35:36.4
01:09:00.43 +58:43:03.8
01:17:42.54 +60:29:21.3
01:31:56.02 +59:26:41.0
01:07:01.76 +59:46:19.6
01:24:16.13 +59:08:33.2
01:12:41.14 +61:18:08.0
01:10:07.90 +57:43:54.9
01:32:22.89 +61:29:14.1
01:41:51.95 +60:08:22.4
01:55:48.24 +58:53:45.3
01:26:16.97 +59:48:45.7
01:41:44.33 +64:14:45.1
01:12:15.26 +58:17:15.8
01:56:12.92 +59:33:49.7
01:51:47.39 +58:37:55.4
01:10:04.80 +57:48:02.7
01:28:32.62 +61:12:20.1
01:15:23.10 +61:11:40.4
01:43:27.43 +58:38:05.3
01:12:59.73 +57:34:07.2
01:11:58.85 +64:42:09.3
01:09:10.40 +58:09:35.6
01:21:22.04 +60:51:44.8
01:07:31.92 +61:28:28.1
01:31:23.04 +59:33:42.4
01:56:43.15 +58:07:17.5
01:44:02.20 +61:52:11.0
01:52:47.75 +58:10:25.4
01:51:09.25 +64:52:45.2
01:34:32.01 +60:30:13.0
01:10:45.61 +64:05:35.1
01:11:56.65 +58:41:05.1
02:15:50.61 +63:12:33.0
01:48:29.79 +60:27:33.3
02:15:03.85 +58:28:53.1
01:23:53.48 +60:53:24.3
01:38:11.78 +65:33:01.0
01:08:59.23 +60:47:20.2
01:10:04.88 +60:32:45.1
01:14:41.46 +58:46:46.2
01:15:11.19 +60:52:41.8
01:10:08.44 +62:43:49.5
01:34:07.12 +60:12:53.2
01:09:22.71 +57:26:30.7
01:21:22.27 +59:45:49.9
01:08:36.84 +60:44:54.0
01:50:58.50 +58:51:12.5
01:59:34.10 +58:19:16.5
01:17:30.55 +57:44:30.7
01:19:29.26 +59:25:22.0
01:33:30.54 +58:02:22.4
01:59:33.87 +63:37:08.5
01:29:25.33 +60:01:31.5
01:24:35.75 +59:32:42.7
01:41:34.38 +59:13:57.5
01:54:05.81 +61:05:12.0
01:13:18.84 +63:56:03.8
02:02:25.13 +64:38:23.5
01:19:08.10 +60:33:39.2
01:54:07.38 +61:05:02.3
01:20:06.59 +60:14:18.5
02:01:06.28 +64:35:47.0
01:38:35.70 +64:48:51.2
01:48:17.77 +60:40:23.1
01:43:17.73 +60:46:50.7
01:32:37.51 +59:38:48.6
01:08:30.34 +61:29:21.9
########### 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 ####
01:40:59.96 +62:28:20.7
01:41:38.74 +63:03:45.9
01:19:08.75 +60:17:19.5
01:34:23.30 +59:34:48.4
01:52:15.83 +65:17:43.8
01:11:35.74 +60:37:33.4
01:06:15.75 +57:53:23.4
01:33:40.62 +59:42:24.0
01:33:12.67 +61:16:55.0
01:57:29.16 +60:09:18.2
01:10:32.20 +59:42:09.4
01:13:00.48 +62:45:32.3
01:23:01.77 +60:35:36.4
01:09:00.43 +58:43:03.8
01:17:42.54 +60:29:21.3
01:31:56.02 +59:26:41.0
01:07:01.76 +59:46:19.6
01:24:16.13 +59:08:33.2
01:12:41.14 +61:18:08.0
01:10:07.90 +57:43:54.9
01:32:22.89 +61:29:14.1
01:41:51.95 +60:08:22.4
01:55:48.24 +58:53:45.3
01:26:16.97 +59:48:45.7
01:41:44.33 +64:14:45.1
01:12:15.26 +58:17:15.8
01:56:12.92 +59:33:49.7
01:51:47.39 +58:37:55.4
01:10:04.80 +57:48:02.7
01:28:32.62 +61:12:20.1
01:15:23.10 +61:11:40.4
01:43:27.43 +58:38:05.3
01:12:59.73 +57:34:07.2
01:11:58.85 +64:42:09.3
01:09:10.40 +58:09:35.6
01:21:22.04 +60:51:44.8
01:07:31.92 +61:28:28.1
01:31:23.04 +59:33:42.4
01:56:43.15 +58:07:17.5
01:44:02.20 +61:52:11.0
01:52:47.75 +58:10:25.4
01:51:09.25 +64:52:45.2
01:34:32.01 +60:30:13.0
01:10:45.61 +64:05:35.1
01:11:56.65 +58:41:05.1
02:15:50.61 +63:12:33.0
01:48:29.79 +60:27:33.3
02:15:03.85 +58:28:53.1
01:23:53.48 +60:53:24.3
01:38:11.78 +65:33:01.0
01:08:59.23 +60:47:20.2
01:10:04.88 +60:32:45.1
01:14:41.46 +58:46:46.2
01:15:11.19 +60:52:41.8
01:10:08.44 +62:43:49.5
01:34:07.12 +60:12:53.2
01:09:22.71 +57:26:30.7
01:21:22.27 +59:45:49.9
01:08:36.84 +60:44:54.0
01:50:58.50 +58:51:12.5
01:59:34.10 +58:19:16.5
01:17:30.55 +57:44:30.7
01:19:29.26 +59:25:22.0
01:33:30.54 +58:02:22.4
01:59:33.87 +63:37:08.5
01:29:25.33 +60:01:31.5
01:24:35.75 +59:32:42.7
01:41:34.38 +59:13:57.5
01:54:05.81 +61:05:12.0
01:13:18.84 +63:56:03.8
02:02:25.13 +64:38:23.5
01:19:08.10 +60:33:39.2
01:54:07.38 +61:05:02.3
01:20:06.59 +60:14:18.5
02:01:06.28 +64:35:47.0
01:38:35.70 +64:48:51.2
01:48:17.77 +60:40:23.1
01:43:17.73 +60:46:50.7
01:32:37.51 +59:38:48.6
01:08:30.34 +61:29:21.9
###################################################################################
01:40:59.96 +62:28:20.7 -- not an asteroid (will add it to exclusion list)
01:41:38.74 +63:03:45.9 -- not an asteroid (will add it to exclusion list)
01:19:08.75 +60:17:19.5 -- not an asteroid (will add it to exclusion list)
01:34:23.30 +59:34:48.4 -- not an asteroid (will add it to exclusion list)
01:52:15.83 +65:17:43.8 -- not an asteroid (will add it to exclusion list)
01:11:35.74 +60:37:33.4 -- not an asteroid (will add it to exclusion list)
01:06:15.75 +57:53:23.4 -- not an asteroid (will add it to exclusion list)
01:33:40.62 +59:42:24.0 -- not an asteroid (will add it to exclusion list)
01:33:12.67 +61:16:55.0 -- not an asteroid (will add it to exclusion list)
01:57:29.16 +60:09:18.2 -- not an asteroid (will add it to exclusion list)
01:10:32.20 +59:42:09.4 -- not an asteroid (will add it to exclusion list)
01:13:00.48 +62:45:32.3 -- not an asteroid (will add it to exclusion list)
01:23:01.77 +60:35:36.4 -- not an asteroid (will add it to exclusion list)
01:09:00.43 +58:43:03.8 -- not an asteroid (will add it to exclusion list)
01:17:42.54 +60:29:21.3 -- not an asteroid (will add it to exclusion list)
01:31:56.02 +59:26:41.0 -- not an asteroid (will add it to exclusion list)
01:07:01.76 +59:46:19.6 -- not an asteroid (will add it to exclusion list)
01:24:16.13 +59:08:33.2 -- not an asteroid (will add it to exclusion list)
01:12:41.14 +61:18:08.0 -- not an asteroid (will add it to exclusion list)
01:10:07.90 +57:43:54.9 -- not an asteroid (will add it to exclusion list)
01:32:22.89 +61:29:14.1 -- not an asteroid (will add it to exclusion list)
01:41:51.95 +60:08:22.4 -- not an asteroid (will add it to exclusion list)
01:55:48.24 +58:53:45.3 -- not an asteroid (will add it to exclusion list)
01:26:16.97 +59:48:45.7 -- not an asteroid (will add it to exclusion list)
01:41:44.33 +64:14:45.1 -- not an asteroid (will add it to exclusion list)
01:12:15.26 +58:17:15.8 -- not an asteroid (will add it to exclusion list)
01:56:12.92 +59:33:49.7 -- not an asteroid (will add it to exclusion list)
01:51:47.39 +58:37:55.4 -- not an asteroid (will add it to exclusion list)
01:10:04.80 +57:48:02.7 -- not an asteroid (will add it to exclusion list)
01:28:32.62 +61:12:20.1 -- not an asteroid (will add it to exclusion list)
01:15:23.10 +61:11:40.4 -- not an asteroid (will add it to exclusion list)
01:43:27.43 +58:38:05.3 -- not an asteroid (will add it to exclusion list)
01:12:59.73 +57:34:07.2 -- not an asteroid (will add it to exclusion list)
01:11:58.85 +64:42:09.3 -- not an asteroid (will add it to exclusion list)
01:09:10.40 +58:09:35.6 -- not an asteroid (will add it to exclusion list)
01:21:22.04 +60:51:44.8 -- not an asteroid (will add it to exclusion list)
01:07:31.92 +61:28:28.1 -- not an asteroid (will add it to exclusion list)
01:31:23.04 +59:33:42.4 -- not an asteroid (will add it to exclusion list)
01:56:43.15 +58:07:17.5 -- not an asteroid (will add it to exclusion list)
01:44:02.20 +61:52:11.0 -- not an asteroid (will add it to exclusion list)
01:52:47.75 +58:10:25.4 -- not an asteroid (will add it to exclusion list)
01:51:09.25 +64:52:45.2 -- not an asteroid (will add it to exclusion list)
01:34:32.01 +60:30:13.0 -- not an asteroid (will add it to exclusion list)
01:10:45.61 +64:05:35.1 -- not an asteroid (will add it to exclusion list)
01:11:56.65 +58:41:05.1 -- not an asteroid (will add it to exclusion list)
02:15:50.61 +63:12:33.0 -- not an asteroid (will add it to exclusion list)
01:48:29.79 +60:27:33.3 -- not an asteroid (will add it to exclusion list)
02:15:03.85 +58:28:53.1 -- not an asteroid (will add it to exclusion list)
01:23:53.48 +60:53:24.3 -- not an asteroid (will add it to exclusion list)
01:38:11.78 +65:33:01.0 -- not an asteroid (will add it to exclusion list)
01:08:59.23 +60:47:20.2 -- not an asteroid (will add it to exclusion list)
01:10:04.88 +60:32:45.1 -- not an asteroid (will add it to exclusion list)
01:14:41.46 +58:46:46.2 -- not an asteroid (will add it to exclusion list)
01:15:11.19 +60:52:41.8 -- not an asteroid (will add it to exclusion list)
01:10:08.44 +62:43:49.5 -- not an asteroid (will add it to exclusion list)
01:34:07.12 +60:12:53.2 -- not an asteroid (will add it to exclusion list)
01:09:22.71 +57:26:30.7 -- not an asteroid (will add it to exclusion list)
01:21:22.27 +59:45:49.9 -- not an asteroid (will add it to exclusion list)
01:08:36.84 +60:44:54.0 -- not an asteroid (will add it to exclusion list)
01:50:58.50 +58:51:12.5 -- not an asteroid (will add it to exclusion list)
01:59:34.10 +58:19:16.5 -- not an asteroid (will add it to exclusion list)
01:17:30.55 +57:44:30.7 -- not an asteroid (will add it to exclusion list)
01:19:29.26 +59:25:22.0 -- not an asteroid (will add it to exclusion list)
01:33:30.54 +58:02:22.4 -- not an asteroid (will add it to exclusion list)
01:59:33.87 +63:37:08.5 -- not an asteroid (will add it to exclusion list)
01:29:25.33 +60:01:31.5 -- not an asteroid (will add it to exclusion list)
01:24:35.75 +59:32:42.7 -- not an asteroid (will add it to exclusion list)
01:41:34.38 +59:13:57.5 -- not an asteroid (will add it to exclusion list)
01:54:05.81 +61:05:12.0 -- not an asteroid (will add it to exclusion list)
01:13:18.84 +63:56:03.8 -- not an asteroid (will add it to exclusion list)
02:02:25.13 +64:38:23.5 -- not an asteroid (will add it to exclusion list)
01:19:08.10 +60:33:39.2 -- not an asteroid (will add it to exclusion list)
01:54:07.38 +61:05:02.3 -- not an asteroid (will add it to exclusion list)
01:20:06.59 +60:14:18.5 -- not an asteroid (will add it to exclusion list)
02:01:06.28 +64:35:47.0 -- not an asteroid (will add it to exclusion list)
01:38:35.70 +64:48:51.2 -- not an asteroid (will add it to exclusion list)
01:48:17.77 +60:40:23.1 -- not an asteroid (will add it to exclusion list)
01:43:17.73 +60:46:50.7 -- not an asteroid (will add it to exclusion list)
01:32:37.51 +59:38:48.6 -- not an asteroid (will add it to exclusion list)
01:08:30.34 +61:29:21.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:06:15.75 +57:53:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:01.76 +59:46:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:31.92 +61:28:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:30.34 +61:29:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:36.84 +60:44:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:59.23 +60:47:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:00.43 +58:43:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:10.40 +58:09:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.71 +57:26:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:04.80 +57:48:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:04.88 +60:32:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:07.90 +57:43:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:08.44 +62:43:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:32.20 +59:42:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:45.61 +64:05:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:35.74 +60:37:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:56.65 +58:41:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:58.85 +64:42:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:15.26 +58:17:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:41.14 +61:18:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:59.73 +57:34:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:00.48 +62:45:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:18.84 +63:56:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:41.46 +58:46:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:11.19 +60:52:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:23.10 +61:11:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:30.55 +57:44:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:42.54 +60:29:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:08.10 +60:33:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:08.75 +60:17:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:29.26 +59:25:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:06.59 +60:14:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:22.04 +60:51:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:22.27 +59:45:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:01.77 +60:35:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:53.48 +60:53:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:16.13 +59:08:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:35.75 +59:32:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:16.97 +59:48:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:32.62 +61:12:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:25.33 +60:01:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:23.04 +59:33:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:56.02 +59:26:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:22.89 +61:29:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:37.51 +59:38:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:12.67 +61:16:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:30.54 +58:02:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:40.62 +59:42:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:07.12 +60:12:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:23.30 +59:34:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:32.01 +60:30:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:11.78 +65:33:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:35.70 +64:48:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:59.96 +62:28:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:34.38 +59:13:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:38.74 +63:03:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:44.33 +64:14:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:51.95 +60:08:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:17.73 +60:46:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:27.43 +58:38:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:02.20 +61:52:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:17.77 +60:40:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:29.79 +60:27:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:58.50 +58:51:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:09.25 +64:52:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:47.39 +58:37:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:15.83 +65:17:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:47.75 +58:10:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:05.81 +61:05:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:07.38 +61:05:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:48.24 +58:53:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:12.92 +59:33:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:43.15 +58:07:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:29.16 +60:09:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:33.87 +63:37:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:34.10 +58:19:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:06.28 +64:35:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:25.13 +64:38:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:03.85 +58:28:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:50.61 +63:12:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:06:15.75 +57:53:23.4 -- not a known variable star
01:07:01.76 +59:46:19.6 -- not a known variable star
01:07:31.92 +61:28:28.1 -- not a known variable star
01:08:30.34 +61:29:21.9 -- a known variable star
01:08:36.84 +60:44:54.0 -- not a known variable star
01:08:59.23 +60:47:20.2 -- not a known variable star
01:09:00.43 +58:43:03.8 -- not a known variable star
01:09:10.40 +58:09:35.6 -- not a known variable star
01:09:22.71 +57:26:30.7 -- not a known variable star
01:10:04.80 +57:48:02.7 -- not a known variable star
01:10:04.88 +60:32:45.1 -- not a known variable star
01:10:07.90 +57:43:54.9 -- not a known variable star
01:10:08.44 +62:43:49.5 -- not a known variable star
01:10:32.20 +59:42:09.4 -- not a known variable star
01:10:45.61 +64:05:35.1 -- not a known variable star
01:11:35.74 +60:37:33.4 -- not a known variable star
01:11:56.65 +58:41:05.1 -- not a known variable star
01:11:58.85 +64:42:09.3 -- a known variable star
01:12:15.26 +58:17:15.8 -- not a known variable star
01:12:41.14 +61:18:08.0 -- not a known variable star
01:12:59.73 +57:34:07.2 -- not a known variable star
01:13:00.48 +62:45:32.3 -- a known variable star
01:13:18.84 +63:56:03.8 -- not a known variable star
01:14:41.46 +58:46:46.2 -- a known variable star
01:15:11.19 +60:52:41.8 -- not a known variable star
01:15:23.10 +61:11:40.4 -- not a known variable star
01:17:30.55 +57:44:30.7 -- a known variable star
01:17:42.54 +60:29:21.3 -- not a known variable star
01:19:08.10 +60:33:39.2 -- not a known variable star
01:19:08.75 +60:17:19.5 -- not a known variable star
01:19:29.26 +59:25:22.0 -- not a known variable star
01:20:06.59 +60:14:18.5 -- not a known variable star
01:21:22.04 +60:51:44.8 -- not a known variable star
01:21:22.27 +59:45:49.9 -- a known variable star
01:23:01.77 +60:35:36.4 -- not a known variable star
01:23:53.48 +60:53:24.3 -- a known variable star
01:24:16.13 +59:08:33.2 -- a known variable star
01:24:35.75 +59:32:42.7 -- a known variable star
01:26:16.97 +59:48:45.7 -- not a known variable star
01:28:32.62 +61:12:20.1 -- not a known variable star
01:29:25.33 +60:01:31.5 -- not a known variable star
01:31:23.04 +59:33:42.4 -- not a known variable star
01:31:56.02 +59:26:41.0 -- not a known variable star
01:32:22.89 +61:29:14.1 -- a known variable star
01:32:37.51 +59:38:48.6 -- not a known variable star
01:33:12.67 +61:16:55.0 -- not a known variable star
01:33:30.54 +58:02:22.4 -- not a known variable star
01:33:40.62 +59:42:24.0 -- a known variable star
01:34:07.12 +60:12:53.2 -- not a known variable star
01:34:23.30 +59:34:48.4 -- a known variable star
01:34:32.01 +60:30:13.0 -- a known variable star
01:38:11.78 +65:33:01.0 -- a known variable star
01:38:35.70 +64:48:51.2 -- not a known variable star
01:40:59.96 +62:28:20.7 -- not a known variable star
01:41:34.38 +59:13:57.5 -- not a known variable star
01:41:38.74 +63:03:45.9 -- a known variable star
01:41:44.33 +64:14:45.1 -- not a known variable star
01:41:51.95 +60:08:22.4 -- not a known variable star
01:43:17.73 +60:46:50.7 -- not a known variable star
01:43:27.43 +58:38:05.3 -- a known variable star
01:44:02.20 +61:52:11.0 -- not a known variable star
01:48:17.77 +60:40:23.1 -- a known variable star
01:48:29.79 +60:27:33.3 -- not a known variable star
01:50:58.50 +58:51:12.5 -- not a known variable star
01:51:09.25 +64:52:45.2 -- a known variable star
01:51:47.39 +58:37:55.4 -- not a known variable star
01:52:15.83 +65:17:43.8 -- not a known variable star
01:52:47.75 +58:10:25.4 -- not a known variable star
01:54:05.81 +61:05:12.0 -- not a known variable star
01:54:07.38 +61:05:02.3 -- not a known variable star
01:55:48.24 +58:53:45.3 -- not a known variable star
01:56:12.92 +59:33:49.7 -- not a known variable star
01:56:43.15 +58:07:17.5 -- not a known variable star
01:57:29.16 +60:09:18.2 -- not a known variable star
01:59:33.87 +63:37:08.5 -- not a known variable star
01:59:34.10 +58:19:16.5 -- a known variable star
02:01:06.28 +64:35:47.0 -- not a known variable star
02:02:25.13 +64:38:23.5 -- a known variable star
02:15:03.85 +58:28:53.1 -- a known variable star
02:15:50.61 +63:12:33.0 -- not a known variable star
Found 59 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
80 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 80 (excluding asteroids and hot pixels, 59 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)2461228.90990256 -observatory V36
07:39:37.17 +17:21:32.7 Mercury (4.1mag)
09:59:11.90 +13:57:00.8 Venus (-4.1mag)
04:15:27.43 +21:02:11.7 Mars (1.3mag)
08:14:00.65 +20:19:47.8 Jupiter (-1.8mag)
00:55:29.90 +03:19:10.0 Saturn (0.7mag)
04:06:39.68 +20:43:30.3 Uranus (5.8mag)
00:17:01.77 +00:20:53.1 Neptune (7.8mag)
20:31:10.93 -23:16:42.9 Pluto (14.4mag)
00:33:23.50 +06:31:01.9 Moon (-10.5mag)
-rw-r--r-- 1 apache apache 362 Jul 7 05:07 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461228.90990256:
08:14:02.18 +20:19:41.5 Io (6.1mag)
08:14:11.60 +20:19:08.8 Europa (6.3mag)
08:13:46.63 +20:20:41.0 Ganymede (5.6mag)
08:14:24.06 +20:18:27.9 Callisto (6.8mag)
08:12:40.54 +20:02:47.2 Himalia (15.7mag)
08:14:01.29 +20:19:46.3 Thebe (16.6mag)
08:12:02.98 +20:07:59.7 Elara (17.6mag)
08:17:27.12 +20:15:32.9 Pasiphae (17.8mag)
08:19:08.42 +20:24:28.6 Carme (19.0mag)
00:55:20.27 +03:19:32.5 Titan (8.5mag)
00:55:32.91 +03:18:56.8 Rhea (9.8mag)
00:55:03.63 +03:18:53.9 Iapetus (11.2mag)
00:55:45.33 +03:19:03.0 Hyperion (14.5mag)
00:55:34.54 +03:16:49.6 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 7 05:08 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461228.90990256:
17:42:24.31 -33:32:20.1 JWST
15:00:30.69 +52:42:40.6 Chandra
10:25:52.57 -57:58:02.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 7 05:08 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461228.90990256 -observatory V36
02:32:02.46 +14:04:12.8 17.9mag P/1996 R2 (Lagerkvist)
18:20:15.36 -34:16:13.8 13.7mag P/2010 H2 (Vales)
06:22:43.38 -68:05:54.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:59:46.29 +32:23:52.6 17.6mag C/2017 K2 (PANSTARRS)
17:03:59.08 +16:03:25.0 18.0mag C/2021 G2 (ATLAS)
01:29:52.07 +01:51:37.0 15.3mag P/2021 N1 (ZTF)
23:01:13.50 +32:16:47.4 17.2mag C/2022 E2 (ATLAS)
06:09:00.97 +26:56:58.8 16.7mag C/2022 N2 (PANSTARRS)
09:52:58.51 +29:54:40.2 16.8mag C/2022 QE78 (ATLAS)
09:07:51.12 +04:56:16.3 17.8mag C/2022 R6 (PANSTARRS)
18:09:02.42 +21:23:47.0 17.9mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:56.26 -11:19:29.1 17.7mag P/2023 B1 (PANSTARRS)
21:52:38.78 +67:37:16.7 17.8mag C/2023 H5 (Lemmon)
16:36:52.83 -09:46:04.7 13.9mag C/2023 R1 (PANSTARRS)
07:55:36.99 +65:33:16.2 17.9mag C/2024 A1 (ATLAS)
07:28:55.10 +29:50:55.7 14.5mag C/2024 E1 (Wierzchos)
15:17:48.98 +15:14:26.8 17.5mag C/2024 G6 (ATLAS)
19:44:58.24 +38:47:23.7 13.8mag C/2024 J3 (ATLAS)
21:50:29.57 +45:32:48.9 17.9mag C/2024 R4 (PANSTARRS)
04:46:50.40 -13:56:15.4 15.8mag C/2024 T5 (ATLAS)
06:32:06.26 +29:33:35.7 18.0mag C/2025 J1 (Borisov)
07:12:12.73 -12:38:26.6 16.3mag C/2025 R3 (PANSTARRS)
09:52:44.43 +22:33:26.4 17.7mag C/2025 V2 (Rankin)
12:43:42.04 +04:03:23.7 17.1mag C/2025 Y1 (ATLAS)
17:00:28.38 +79:01:25.8 17.4mag C/2026 A2 (Bok)
02:43:00.22 +45:06:27.0 16.6mag C/2026 B2 (Sun-Gao)
11:23:41.98 +03:59:48.1 16.9mag A/2026 E1
21:14:19.09 -14:05:02.1 7.4mag 10P/Tempel
11:12:06.92 -01:46:00.3 16.1mag 29P/Schwassmann-Wachmann
03:55:53.67 +29:13:41.6 17.8mag 47P/Ashbrook-Jackson
10:01:54.94 +14:56:39.3 17.0mag 63P/Wild
00:46:58.99 -05:08:19.5 15.6mag 65P/Gunn
08:17:42.68 +34:20:14.3 17.8mag 76P/West-Kohoutek-Ikemura
04:20:15.62 +20:00:35.2 13.7mag 78P/Gehrels
02:17:26.36 +10:11:11.6 16.2mag 88P/Howell
06:26:40.81 +30:41:06.3 15.6mag 93P/Lovas
04:11:30.35 +30:58:13.9 16.9mag 114P/Wiseman-Skiff
08:01:29.72 +31:00:57.2 15.3mag 123P/West-Hartley
10:42:40.20 +02:23:21.4 16.8mag 124P/Mrkos
04:46:58.65 +20:43:14.2 16.3mag 128P/Shoemaker-Holt
05:30:40.11 +19:43:35.4 17.8mag 131P/Mueller
00:00:39.29 +02:48:37.3 18.0mag 139P/Vaisala-Oterma
07:02:25.37 +17:38:23.5 15.2mag 141P-D/Machholz
03:15:30.67 -21:21:46.3 15.6mag 161P/Hartley-IRAS
05:22:29.30 +33:16:27.5 15.3mag 162P/SidingSpring
19:11:06.89 +13:22:54.9 15.0mag 169P/NEAT
01:33:54.12 +07:14:46.4 17.7mag 220P/McNaught
16:36:31.39 -08:16:58.7 17.0mag 235P/LINEAR
08:39:02.41 +33:33:45.7 17.9mag 240P/NEAT
20:43:10.57 -48:53:26.0 17.8mag 259P/Garradd
01:51:06.28 +10:43:02.0 15.7mag 260P/McNaught
05:28:20.12 +36:35:00.9 17.4mag 295P/LINEAR
15:06:51.18 +06:18:38.0 17.6mag 391P/Kowalski
08:31:58.41 +19:47:36.6 17.9mag 450P/LONEOS
07:47:07.34 +39:27:30.3 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 7 05:08 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
16:41:15.63 +39:17:14.70 2026-06-26.38 16.07
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
16:41:15.63 +39:17:14.70 2026-06-26.38 16.07
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 2026-04-9.14 13.64
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
-rw-r--r-- 1 apache apache 5.6K Jul 7 05:07 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 7 05:07 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:36:16.312 -33:07:23.31 AT 2026rmf 2026-06-22.58 20.67
20:43:31.883 -06:33:13.40 AT 2026rme 2026-06-22.44 21.69
09:40:14.549 -04:56:19.06 AT 2026rmd 2026-02-14.41 21.59
13:59:57.150 -09:03:11.62 AT 2026rmc 2026-02-17.61 20.73
12:25:30.012 -26:12:13.68 AT 2026rmb 2026-01-27.58 21.09
03:21:09.438 +39:25:53.03 AT 2026rma 2026-01-13.29 20.19
13:07:11.418 +13:39:38.85 AT 2026rlz 2026-02-25.47 20.51
03:01:07.569 -26:13:29.83 AT 2026rly 2026-01-09.24 20.54
17:01:46.968 -17:03:38.47 AT 2026rlx 2026-07-04.18 18.537
15:04:30.380 -39:18:48.60 AT 2026rlw 2026-07-04.31 18.9
21:26:04.454 -52:53:31.58 AT 2026rlv 2026-07-04.01 18.538
09:44:11.615 +04:40:29.15 AT 2026rlu 2026-04-19.27 20.88
12:57:25.723 -07:44:47.85 AT 2026rlt 2026-04-22.35 20.53
11:52:32.131 -13:45:09.94 AT 2026rls 2026-04-22.31 21.02
16:41:34.520 +44:47:03.76 AT 2026rlr 2026-04-23.49 21.03
11:22:02.700 -24:23:51.28 AT 2026rlq 2026-05-07.27 20.73
13:17:29.523 +09:10:51.61 AT 2026rlp 2026-05-21.26 20.85
20:21:54.334 -21:13:51.37 AT 2026rlo 2026-05-20.57 19.91
20:13:59.295 -23:24:43.54 AT 2026rln 2026-05-20.56 20.51
20:30:30.579 -12:41:46.85 AT 2026rlm 2026-05-21.56 19.73
-rw-r--r-- 1 apache apache 29K Jul 7 05:07 tns_transients_list.txt
