This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY
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 04 28.4429 2461158.9429 11.81 01:43:20.59 +61:14:37.2
129.13446 -1.00145 galactic Cas Second-epoch detections are separated by 1.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:43:20.59 +61:14:37.2 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.037 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:20.59 +61:14:37.2: 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 01:43:20.59 +61:14:37.2: 14.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 43 20.59 +61 14 37.2 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,2461158.9429,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260428.4429 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.51 01:22:33.09 +60:44:41.8
126.72639 -1.89737 galactic Cas Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:22:33.09 +60:44:41.8 (user input) | T | P | (position from user input) J-Ks=1.158+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:33.09 +60:44:41.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:33.09 +60:44:41.8: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 04 28.4429* 01 22 33.09 +60 44 41.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260428.4429 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.74 01:12:30.20 +62:02:37.7
125.39825 -0.72702 galactic Cas Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:30.20 +62:02:37.7 (user input) | T | P | (position from user input) J-Ks=0.423+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:30.20 +62:02:37.7: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:30.20 +62:02:37.7: 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 04 28.4429* 01 12 30.20 +62 02 37.7 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
target,2461158.9429,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.59 02:00:50.08 +62:37:50.5
130.81207 0.82549 galactic Cas Second-epoch detections are separated by 1.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 508846216033919488 | 02:00:47.41 +62:37:49.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.903+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:50.08 +62:37:50.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:50.08 +62:37:50.5: 13.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 04 28.4429* 02 00 50.08 +62 37 50.5 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
Gaia DR3 508846216033919488,2461158.9429,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508846216033919488 20260428.4429 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 04 28.4429 2461158.9429 11.44 01:55:46.55 +57:57:43.0
131.40267 -3.84777 galactic Per Second-epoch detections are separated by 1.1" and 6.5 pix
The object was found in VSX17" ZTF J015546.41+575800.1
Type: RS
# Max. Min./Amp. JD0 Period
13.450 r Y 0.033 r 2458379.91220 0.825740500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:46.55 +57:57:43.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:46.55 +57:57:43.0: 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 04 28.4429* 01 55 46.55 +57 57 43.0 11.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J015546.41+575800.1,2461158.9429,11.44,0.05,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
ZTF J015546.41+575800.1 20260428.4429 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 04 28.4429 2461158.9429 11.65 01:59:11.69 +65:05:59.3
129.98908 3.16058 galactic Cas Second-epoch detections are separated by 1.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:11.69 +65:05:59.3 (user input) | T | P | (position from user input) J-Ks=1.024+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:11.69 +65:05:59.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:11.69 +65:05:59.3: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 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 04 28.4429* 01 59 11.69 +65 05 59.3 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.48 01:47:51.34 +61:11:12.6
129.67766 -0.94382 galactic Cas Second-epoch detections are separated by 1.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511214048684134528 | 01:47:54.00 +61:10:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.225+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:51.34 +61:11:12.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:51.34 +61:11:12.6: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 47 51.34 +61 11 12.6 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 511214048684134528,2461158.9429,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511214048684134528 20260428.4429 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.54 01:13:01.23 +61:00:59.2
125.54468 -1.74577 galactic Cas Second-epoch detections are separated by 2.5" and 6.7 pix
The object was found in VSX 4" Gaia DR3 522455906553654144
Type:
# Max. Min./Amp. JD0 Period
16.000 G 16.860 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:01.23 +61:00:59.2: 12.54 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:01.23 +61:00:59.2: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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 04 28.4429* 01 13 01.23 +61 00 59.2 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 522455906553654144,2461158.9429,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522455906553654144 20260428.4429 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.48 01:37:23.70 +59:20:12.8
128.77029 -3.01291 galactic Cas Second-epoch detections are separated by 1.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:37:23.70 +59:20:12.8 (user input) | T | P | (position from user input) J-Ks=0.300+/-0.042 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:23.70 +59:20:12.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:23.70 +59:20:12.8: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 37 23.70 +59 20 12.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260428.4429 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.51 01:23:56.46 +62:15:25.4
126.70465 -0.37637 galactic Cas Second-epoch detections are separated by 3.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:23:56.46 +62:15:25.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:56.46 +62:15:25.4: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:56.46 +62:15:25.4: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 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 04 28.4429* 01 23 56.46 +62 15 25.4 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
target,2461158.9429,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260428.4429 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.60 01:12:41.33 +61:18:07.0
125.48108 -1.46458 galactic Cas Second-epoch detections are separated by 2.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:41.33 +61:18:07.0 (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 01:12:41.33 +61:18:07.0: 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 01:12:41.33 +61:18:07.0: 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 04 28.4429* 01 12 41.33 +61 18 07.0 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
target,2461158.9429,11.60,0.05,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
target 20260428.4429 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 04 28.4429 2461158.9429 11.51 01:10:12.01 +59:17:25.2
125.32981 -3.49403 galactic Cas Second-epoch detections are separated by 1.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.5672+59.2942 | 01:10:12.01 +59:17:25.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.414+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:12.01 +59:17:25.2: 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 01:10:12.01 +59:17:25.2: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 10 12.01 +59 17 25.2 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
ATO J017.5672+59.2942,2461158.9429,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.5672+59.2942 20260428.4429 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.31 02:00:06.54 +59:00:31.6
131.68364 -2.69117 galactic Cas Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507781618204489856 | 02:00:05.90 +59:00:52.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.381+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:06.54 +59:00:31.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:06.54 +59:00:31.6: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 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 04 28.4429* 02 00 06.54 +59 00 31.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507781618204489856,2461158.9429,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507781618204489856 20260428.4429 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.39 01:24:54.87 +59:41:46.2
127.14907 -2.90119 galactic Cas Second-epoch detections are separated by 3.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:24:54.87 +59:41:46.2 (user input) | T | P | (position from user input) J-Ks=0.217+/-0.043 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:54.87 +59:41:46.2: 13.18 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:54.87 +59:41:46.2: 13.94 +/- 0.06 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 04 28.4429* 01 24 54.87 +59 41 46.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.51 01:08:39.00 +60:32:41.9
125.04802 -2.25604 galactic Cas Second-epoch detections are separated by 1.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:39.00 +60:32:41.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:39.00 +60:32:41.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:39.00 +60:32:41.9: 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 04 28.4429* 01 08 39.00 +60 32 41.9 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,2461158.9429,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260428.4429 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.28 01:12:09.70 +58:47:54.0
125.61967 -3.96522 galactic Cas Second-epoch detections are separated by 0.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:09.70 +58:47:54.0 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:09.70 +58:47:54.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:09.70 +58:47:54.0: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 12 09.70 +58 47 54.0 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,2461158.9429,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260428.4429 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.12 01:14:01.30 +57:40:45.9
125.95887 -5.05954 galactic Cas Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:14:01.30 +57:40:45.9 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:01.30 +57:40:45.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:01.30 +57:40:45.9: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 14 01.30 +57 40 45.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.16 01:07:39.25 +59:59:18.1
124.96085 -2.81949 galactic Cas Second-epoch detections are separated by 1.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:39.25 +59:59:18.1 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.25 +59:59:18.1: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.25 +59:59:18.1: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 04 28.4429* 01 07 39.25 +59 59 18.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 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 04 28.4429 2461158.9429 11.22 01:33:01.59 +59:16:33.9
128.23036 -3.16715 galactic Cas Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J013303.78+591550.3 | 01:33:03.78 +59:15:50.3 (Gaia DR3) | SRS (local) | 16.088000000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:01.59 +59:16:33.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:01.59 +59:16:33.9: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 33 01.59 +59 16 33.9 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
ASASSN-V J013303.78+591550.3,2461158.9429,11.22,0.05,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 J013303.78+591550.3 20260428.4429 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 04 28.4429 2461158.9429 11.10 01:43:27.28 +59:35:12.7
129.47976 -2.62197 galactic Cas Second-epoch detections are separated by 1.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509512417001105664 | 01:43:27.86 +59:35:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9 1955ApJS....2..123F LF 5 +59 162 J-Ks=0.984+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:27.28 +59:35:12.7: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.28 +59:35:12.7: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 43 27.28 +59 35 12.7 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 509512417001105664,2461158.9429,11.10,0.05,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 509512417001105664 20260428.4429 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 04 28.4429 2461158.9429 11.19 01:43:27.30 +58:38:07.8
129.67088 -3.55399 galactic Cas Second-epoch detections are separated by 0.7" and 6.5 pix
The object was found in VSX 2" 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 01:43:27.30 +58:38:07.8: 13.00 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.30 +58:38:07.8: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 43 27.30 +58 38 07.8 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
Gaia DR3 506084487648397824,2461158.9429,11.19,0.05,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 506084487648397824 20260428.4429 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 04 28.4429 2461158.9429 11.13 01:26:05.48 +59:01:14.5
127.38725 -3.55096 galactic Cas Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.5231+59.0209 | 01:26:05.48 +59:01:14.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.48 +59:01:14.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.48 +59:01:14.5: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 04 28.4429* 01 26 05.48 +59 01 14.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.5231+59.0209,2461158.9429,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.5231+59.0209 20260428.4429 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.02 01:56:43.16 +58:07:16.3
131.48413 -3.66246 galactic Cas Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:43.16 +58:07:16.3 (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 01:56:43.16 +58:07:16.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:43.16 +58:07:16.3: 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 04 28.4429* 01 56 43.16 +58 07 16.3 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,2461158.9429,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 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 04 28.4429 2461158.9429 11.06 01:07:34.94 +57:33:09.7
125.10523 -5.25091 galactic Cas Second-epoch detections are separated by 1.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:34.94 +57:33:09.7 (user input) | T | P | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.856+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:34.94 +57:33:09.7: 12.12 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:34.94 +57:33:09.7: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 07 34.94 +57 33 09.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.13 01:07:41.68 +60:54:05.7
124.90821 -1.90777 galactic Cas Second-epoch detections are separated by 1.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:41.68 +60:54:05.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:41.68 +60:54:05.7: 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 01:07:41.68 +60:54:05.7: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 07 41.68 +60 54 05.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.19 01:10:43.79 +60:59:19.6
125.27001 -1.79536 galactic Cas Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:10:43.79 +60:59:19.6 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:43.79 +60:59:19.6: 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 01:10:43.79 +60:59:19.6: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 10 43.79 +60 59 19.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 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 04 28.4429 2461158.9429 11.05 01:15:23.08 +61:11:40.9
125.81352 -1.54300 galactic Cas Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 01:15:23.08 +61:11:40.9: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:23.08 +61:11:40.9: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 15 23.08 +61 11 40.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510546374554030464,2461158.9429,11.05,0.05,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 510546374554030464 20260428.4429 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 04 28.4429 2461158.9429 10.89 01:42:44.41 +58:39:00.7
129.57664 -3.55812 galactic Cas Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506082013747225856 | 01:42:46.84 +58:39:03.8 (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 01:42:44.41 +58:39:00.7: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:44.41 +58:39:00.7: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 04 28.4429* 01 42 44.41 +58 39 00.7 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506082013747225856,2461158.9429,10.89,0.05,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 506082013747225856 20260428.4429 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 04 28.4429 2461158.9429 10.92 01:49:15.97 +59:14:38.1
130.27567 -2.80080 galactic Cas Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506536352570768768 | 01:49:14.31 +59:14:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.811+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:15.97 +59:14:38.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:15.97 +59:14:38.1: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 49 15.97 +59 14 38.1 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 506536352570768768,2461158.9429,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506536352570768768 20260428.4429 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.78 01:19:23.99 +58:26:39.7
126.59360 -4.22845 galactic Cas Second-epoch detections are separated by 2.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413883771873740416 | 01:19:25.94 +58:26:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1951UppAn...2j...1B NGC 457 191 J-Ks=0.329+/-0.040 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:23.99 +58:26:39.7: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:23.99 +58:26:39.7: 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 04 28.4429* 01 19 23.99 +58 26 39.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413883771873740416,2461158.9429,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413883771873740416 20260428.4429 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.85 01:31:22.92 +59:33:42.3
127.97841 -2.91805 galactic Cas Second-epoch detections are separated by 2.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J022.8294+59.5638 | 01:31:22.92 +59:33:42.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.833+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:22.92 +59:33:42.3: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:22.92 +59:33:42.3: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 31 22.92 +59 33 42.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.8294+59.5638,2461158.9429,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.8294+59.5638 20260428.4429 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.78 01:25:15.25 +64:40:33.2
126.53961 2.04128 galactic Cas Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512840196327698304 | 01:25:16.38 +64:40:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.479+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:15.25 +64:40:33.2: 11.18 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:15.25 +64:40:33.2: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 25 15.25 +64 40 33.2 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 512840196327698304,2461158.9429,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512840196327698304 20260428.4429 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.62 02:13:47.56 +58:44:00.0
133.45805 -2.44513 galactic Per Second-epoch detections are separated by 1.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J033.4383+58.7294 | 02:13:47.56 +58:44:00.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.232+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.56 +58:44:00.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.56 +58:44:00.0: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 02 13 47.56 +58 44 00.0 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J033.4383+58.7294,2461158.9429,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J033.4383+58.7294 20260428.4429 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.71 01:09:46.02 +58:12:06.5
125.35233 -4.58378 galactic Cas Second-epoch detections are separated by 1.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:09:46.02 +58:12:06.5 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.229+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:46.02 +58:12:06.5: 12.88 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:46.02 +58:12:06.5: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 04 28.4429* 01 09 46.02 +58 12 06.5 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,10.71,0.05,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
target 20260428.4429 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 04 28.4429 2461158.9429 10.50 01:14:45.34 +60:30:04.0
125.80081 -2.24068 galactic Cas Second-epoch detections are separated by 0.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510401067222116992 | 01:14:43.22 +60:30:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5: 1935BSD...C01....0S BSD 8- 705 J-Ks=0.606+/-0.039 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:45.34 +60:30:04.0: 13.15 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:45.34 +60:30:04.0: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 04 28.4429* 01 14 45.34 +60 30 04.0 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510401067222116992,2461158.9429,10.50,0.05,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
Gaia DR3 510401067222116992 20260428.4429 10.50CV 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 04 28.4429 2461158.9429 10.35 01:12:40.98 +61:20:38.9
125.47690 -1.42258 galactic Cas Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 522563173351220736 | 01:12:36.96 +61:20:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.300+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:40.98 +61:20:38.9: 12.65 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:40.98 +61:20:38.9: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 12 40.98 +61 20 38.9 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522563173351220736,2461158.9429,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 522563173351220736 20260428.4429 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.34 01:07:57.19 +63:37:32.5
124.76498 0.81274 galactic Cas Second-epoch detections are separated by 1.9" and 6.1 pix
The object was found in VSX21" V1064 Cas
Type: EW
# Max. Min./Amp. JD0 Period
11.300 R1 11.800 R1 2451349.91900 0.457606000000 B2
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 01:07:57.19 +63:37:32.5: 10.67 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:57.19 +63:37:32.5: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 07 57.19 +63 37 32.5 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1064 Cas,2461158.9429,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1064 Cas 20260428.4429 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.10 01:15:55.97 +58:23:29.5
126.14617 -4.32727 galactic Cas Second-epoch detections are separated by 1.1" and 6.6 pix
The object was found in VSX 0" Gaia DR3 413870985743610496
Type: SR|M
# Max. Min./Amp. JD0 Period
11.790 G 12.050 G 429.500000000000 M
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 01:15:55.97 +58:23:29.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:55.97 +58:23:29.5: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 15 55.97 +58 23 29.5 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413870985743610496,2461158.9429,10.10,0.05,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 413870985743610496 20260428.4429 10.10CV 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 04 28.4429 2461158.9429 10.05 01:55:14.56 +59:32:02.5
130.94832 -2.34098 galactic Cas Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506368711405378560 | 01:55:13.64 +59:31:39.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.224+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:14.56 +59:32:02.5: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:14.56 +59:32:02.5: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 55 14.56 +59 32 02.5 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506368711405378560,2461158.9429,10.05,0.05,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 506368711405378560 20260428.4429 10.05CV 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 04 28.4429 2461158.9429 10.16 01:35:24.92 +60:39:14.9
128.29739 -1.75866 galactic Cas Second-epoch detections are separated by 2.0" and 6.3 pix
The object was found in VSX 7" Gaia DR3 509819081975016960
Type: S
# Max. Min./Amp. JD0 Period
17.140 G 17.450 G O
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:24.92 +60:39:14.9: 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 01:35:24.92 +60:39:14.9: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 35 24.92 +60 39 14.9 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509819081975016960,2461158.9429,10.16,0.05,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 509819081975016960 20260428.4429 10.16CV 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 04 28.4429 2461158.9429 10.07 01:57:04.02 +64:41:41.6
129.87429 2.71143 galactic Cas Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 518047655195762560 | 01:57:03.69 +64:42:01.2 (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 01:57:04.02 +64:41:41.6: 12.70 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:04.02 +64:41:41.6: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 57 04.02 +64 41 41.6 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 518047655195762560,2461158.9429,10.07,0.05,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 518047655195762560 20260428.4429 10.07CV 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 04 28.4429 2461158.9429 9.89 01:15:16.84 +57:28:04.4
126.14682 -5.25495 galactic Cas Second-epoch detections are separated by 2.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413443898501160704 | 01:15:18.56 +57:27:47.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.238+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:16.84 +57:28:04.4: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:16.84 +57:28:04.4: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 15 16.84 +57 28 04.4 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413443898501160704,2461158.9429,9.89,0.05,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 413443898501160704 20260428.4429 9.89CV 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 04 28.4429 2461158.9429 9.92 01:20:24.41 +59:10:24.7
126.64272 -3.48934 galactic Cas Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J020.1204+59.1623 | 01:20:25.01 +59:10:05.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.296+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:24.41 +59:10:24.7: 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 01:20:24.41 +59:10:24.7: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 20 24.41 +59 10 24.7 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J020.1204+59.1623,2461158.9429,9.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J020.1204+59.1623 20260428.4429 9.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 9.67 01:19:48.74 +61:38:15.1
126.29561 -1.04877 galactic Cas Second-epoch detections are separated by 0.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510901241928240128 | 01:19:47.76 +61:38:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2: 1935BSD...C01....0S BSD 8-1789/90 J-Ks=0.282+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:48.74 +61:38:15.1: 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 01:19:48.74 +61:38:15.1: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 19 48.74 +61 38 15.1 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510901241928240128,2461158.9429,9.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 510901241928240128 20260428.4429 9.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 9.56 01:25:56.60 +59:35:11.9
127.29255 -2.99265 galactic Cas Second-epoch detections are separated by 2.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510075336901717632 | 01:25:55.70 +59:34:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +59 169 J-Ks=0.194+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:56.60 +59:35:11.9: 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 01:25:56.60 +59:35:11.9: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 25 56.60 +59 35 11.9 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510075336901717632,2461158.9429,9.56,0.05,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 510075336901717632 20260428.4429 9.56CV 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 04 28.4429 2461158.9429 9.12 01:16:00.98 +62:41:57.8
125.74593 -0.03799 galactic Cas Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 523030538810955648 | 01:16:01.09 +62:41:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1960IzKry..24..160B [B60] +62 89 J-Ks=0.197+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:00.98 +62:41:57.8: 11.19 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:00.98 +62:41:57.8: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 16 00.98 +62 41 57.8 9.1 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 523030538810955648,2461158.9429,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523030538810955648 20260428.4429 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 8.91 02:13:07.47 +58:04:48.1
133.57896 -3.09311 galactic Per Second-epoch detections are separated by 0.5" and 6.1 pix
The object was found in VSX 0" UX Per
Type: DCEP
# Max. Min./Amp. JD0 Period
11.020 V 12.070 V 2437402.94500 4.565815000000 F5-G3
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 02:13:07.47 +58:04:48.1: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:07.47 +58:04:48.1: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 02 13 07.47 +58 04 48.1 8.9 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
UX Per,2461158.9429,8.91,0.05,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
UX Per 20260428.4429 8.91CV 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 04 28.4429 2461158.9429 9.59 01:19:11.07 +58:20:31.4
126.57658 -4.33321 galactic Cas Second-epoch detections are separated by 0.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413877380962478336 | 01:19:10.27 +58:20:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B1 1951UppAn...2j...1B NGC 457 120 J-Ks=0.002+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:11.07 +58:20:31.4: 12.87 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:11.07 +58:20:31.4: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 19 11.07 +58 20 31.4 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413877380962478336,2461158.9429,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413877380962478336 20260428.4429 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.15 01:25:42.74 +65:40:08.9
126.45624 3.03220 galactic Cas Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 525281273472220544 | 01:25:45.20 +65:40:30.5 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE J-Ks=0.362+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:42.74 +65:40:08.9: 12.17 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:42.74 +65:40:08.9: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 25 42.74 +65 40 08.9 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 525281273472220544,2461158.9429,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 525281273472220544 20260428.4429 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.20 01:18:14.21 +61:44:36.6
126.09854 -0.96337 galactic Cas Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:14.21 +61:44:36.6 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:14.21 +61:44:36.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:14.21 +61:44:36.6: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 18 14.21 +61 44 36.6 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,10.20,0.05,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 20260428.4429 10.20CV 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 04 28.4429 2461158.9429 10.36 02:15:40.50 +62:14:22.0
132.56818 0.95411 galactic Cas Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 513816631370458752 | 02:15:45.36 +62:14:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1932MeUpp..55....1S BD+61 394 J-Ks=0.205+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:40.50 +62:14:22.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:40.50 +62:14:22.0: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 02 15 40.50 +62 14 22.0 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 513816631370458752,2461158.9429,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 513816631370458752 20260428.4429 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.51 02:06:39.03 +64:09:28.7
131.01602 2.47311 galactic Cas Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:06:39.03 +64:09:28.7 (user input) | T | P | (position from user input) J-Ks=0.859+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:06:39.03 +64:09:28.7: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:06:39.03 +64:09:28.7: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 02 06 39.03 +64 09 28.7 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260428.4429 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.66 02:20:52.98 +63:53:40.1
132.57984 2.71094 galactic Cas Second-epoch detections are separated by 1.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 515115223323344128 | 02:20:49.36 +63:53:39.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:52.98 +63:53:40.1: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:52.98 +63:53:40.1: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 04 28.4429* 02 20 52.98 +63 53 40.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 515115223323344128,2461158.9429,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 515115223323344128 20260428.4429 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.49 01:44:32.31 +58:45:36.4
129.78365 -3.40344 galactic Cas Second-epoch detections are separated by 0.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506461620135299584 | 01:44:30.78 +58:46:10.9 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B8: 1955ApJS....2..123F LF 5 +58 58 J-Ks=0.189+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:32.31 +58:45:36.4: 13.32 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:32.31 +58:45:36.4: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 04 28.4429* 01 44 32.31 +58 45 36.4 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506461620135299584,2461158.9429,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506461620135299584 20260428.4429 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.56 02:11:23.05 +61:21:06.1
132.36350 -0.04747 galactic Cas Second-epoch detections are separated by 1.2" and 5.7 pix
The object was found in VSX19" Gaia DR3 507740455237382016
Type: ROT
# Max. Min./Amp. JD0 Period
14.500 G 14.530 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:23.05 +61:21:06.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:23.05 +61:21:06.1: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 04 28.4429* 02 11 23.05 +61 21 06.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507740455237382016,2461158.9429,10.56,0.05,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 507740455237382016 20260428.4429 10.56CV 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 04 28.4429 2461158.9429 10.79 02:16:36.25 +64:57:46.7
131.78895 3.56603 galactic Cas Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:16:36.25 +64:57:46.7 (user input) | T | P | (position from user input) J-Ks=0.520+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:36.25 +64:57:46.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:36.25 +64:57:46.7: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 04 28.4429* 02 16 36.25 +64 57 46.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.88 01:39:24.65 +63:23:54.6
128.27172 1.02521 galactic Cas Second-epoch detections are separated by 1.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512471653773856768 | 01:39:21.54 +63:23:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.054 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:24.65 +63:23:54.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:24.65 +63:23:54.6: 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 04 28.4429* 01 39 24.65 +63 23 54.6 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512471653773856768,2461158.9429,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512471653773856768 20260428.4429 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.67 02:11:50.19 +59:02:57.3
133.11969 -2.22299 galactic Per Second-epoch detections are separated by 2.2" and 5.9 pix
The object was found in VSX 2" NSVS J0211521+590234
Type: SR
# Max. Min./Amp. JD0 Period
13.888 r Y 0.567 r 2458346.14140 174.387018500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:50.19 +59:02:57.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:50.19 +59:02:57.3: 14.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 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 04 28.4429* 02 11 50.19 +59 02 57.3 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0211521+590234,2461158.9429,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0211521+590234 20260428.4429 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.91 01:19:41.51 +62:51:06.1
126.14849 0.15654 galactic Cas Second-epoch detections are separated by 1.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:19:41.51 +62:51:06.1 (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 01:19:41.51 +62:51:06.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:41.51 +62:51:06.1: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 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 04 28.4429* 01 19 41.51 +62 51 06.1 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
target,2461158.9429,10.91,0.05,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
target 20260428.4429 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 04 28.4429 2461158.9429 10.90 01:40:34.78 +60:45:54.2
128.89908 -1.53609 galactic Cas Second-epoch detections are separated by 1.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.1283+60.7735 | 01:40:28.84 +60:45:47.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:34.78 +60:45:54.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:34.78 +60:45:54.2: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 40 34.78 +60 45 54.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.1283+60.7735,2461158.9429,10.90,0.05,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
ATO J025.1283+60.7735 20260428.4429 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 04 28.4429 2461158.9429 10.94 01:46:38.46 +60:07:33.0
129.76011 -2.01203 galactic Cas Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.6591+60.1406 | 01:46:39.63 +60:07:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.46 +60:07:33.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.46 +60:07:33.0: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 04 28.4429* 01 46 38.46 +60 07 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
ATO J026.6591+60.1406,2461158.9429,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.6591+60.1406 20260428.4429 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.85 01:58:04.34 +57:58:50.4
131.69330 -3.75310 galactic Per Second-epoch detections are separated by 3.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.5229+57.9688 | 01:58:04.34 +57:58:50.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.847+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:04.34 +57:58:50.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:04.34 +57:58:50.4: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 04 28.4429* 01 58 04.34 +57 58 50.4 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J029.5229+57.9688,2461158.9429,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J029.5229+57.9688 20260428.4429 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 10.90 01:44:46.18 +57:50:37.1
130.00198 -4.29416 galactic Cas Second-epoch detections are separated by 2.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.1759+57.8560 | 01:44:41.39 +57:50:49.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3 1928AnHar.100...49C HD 236851
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:46.18 +57:50:37.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:46.18 +57:50:37.1: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 44 46.18 +57 50 37.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.1759+57.8560,2461158.9429,10.90,0.05,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
ATO J026.1759+57.8560 20260428.4429 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 04 28.4429 2461158.9429 10.96 01:38:33.99 +58:07:23.8
129.13884 -4.17938 galactic Cas Second-epoch detections are separated by 0.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.6134+58.1331 | 01:38:30.85 +58:07:55.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K2III 1932MeUpp..55....1S BD+57 352 J-Ks=0.819+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:33.99 +58:07:23.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:33.99 +58:07:23.8: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 38 33.99 +58 07 23.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.6134+58.1331,2461158.9429,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.6134+58.1331 20260428.4429 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.04 02:02:41.62 +59:59:00.2
131.73882 -1.66434 galactic Cas Second-epoch detections are separated by 2.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507929158919835264 | 02:02:37.35 +59:58:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB 1928MeUpp..37....1S BD+59 388 J-Ks=0.339+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:41.62 +59:59:00.2: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:41.62 +59:59:00.2: 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 04 28.4429* 02 02 41.62 +59 59 00.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507929158919835264,2461158.9429,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507929158919835264 20260428.4429 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 04 28.4429 2461158.9429 11.05 01:36:16.29 +60:12:24.4
128.47827 -2.18128 galactic Cas Second-epoch detections are separated by 2.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509768332640107392 | 01:36:16.56 +60:11:46.2 (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 01:36:16.29 +60:12:24.4: 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 01:36:16.29 +60:12:24.4: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 04 28.4429* 01 36 16.29 +60 12 24.4 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 509768332640107392,2461158.9429,11.05,0.05,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 509768332640107392 20260428.4429 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 04 28.4429 2461158.9429 10.88 02:10:23.84 +60:01:13.5
132.65101 -1.35294 galactic Cas Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:10:23.84 +60:01:13.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.329+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:23.84 +60:01:13.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:23.84 +60:01:13.5: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 04 28.4429* 02 10 23.84 +60 01 13.5 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.21 01:31:48.20 +64:21:56.8
127.28155 1.83546 galactic Cas Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.20 +64:21:56.8 (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 01:31:48.20 +64:21:56.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.20 +64:21:56.8: 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 04 28.4429* 01 31 48.20 +64 21 56.8 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,2461158.9429,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.10 01:32:05.68 +61:59:25.7
127.68585 -0.50543 galactic Cas Second-epoch detections are separated by 1.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510798197068398848 | 01:32:04.51 +61:59:00.7 (Gaia DR3) | DSCT/GDOR (local) | A (local) | Gaia3var=VARIABLE SpType: F5 1960IzKry..24..160B [B60] +61 281 J-Ks=0.127+/-0.036 (A)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:05.68 +61:59:25.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:05.68 +61:59:25.7: 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 04 28.4429* 01 32 05.68 +61 59 25.7 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 510798197068398848,2461158.9429,11.10,0.05,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 510798197068398848 20260428.4429 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 04 28.4429 2461158.9429 11.23 01:48:29.91 +60:27:35.3
129.91278 -1.63625 galactic Cas Second-epoch detections are separated by 6.3" and 5.1 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 | 01:48:29.91 +60:27:35.3 (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 01:48:29.91 +60:27:35.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:29.91 +60:27:35.3: 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 04 28.4429* 01 48 29.91 +60 27 35.3 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
target,2461158.9429,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.32 01:50:39.66 +62:00:55.2
129.81882 -0.06193 galactic Cas Second-epoch detections are separated by 3.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511356332360621440 | 01:50:34.89 +62:00:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1955ApJS....2..123F LF 5 +61 158
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.66 +62:00:55.2: 13.54 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.66 +62:00:55.2: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 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 04 28.4429* 01 50 39.66 +62 00 55.2 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 511356332360621440,2461158.9429,11.32,0.05,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 511356332360621440 20260428.4429 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 04 28.4429 2461158.9429 11.11 01:59:05.82 +59:55:35.2
131.31975 -1.83887 galactic Cas Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:05.82 +59:55:35.2 (user input) | T | P | (position from user input) J-Ks=0.818+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:05.82 +59:55:35.2: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:05.82 +59:55:35.2: 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 04 28.4429* 01 59 05.82 +59 55 35.2 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
target,2461158.9429,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.21 01:19:28.88 +59:54:38.2
126.44435 -2.76975 galactic Cas Second-epoch detections are separated by 1.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510323036254643328 | 01:19:24.22 +59:54:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B6 1935BSD...C01....0S BSD 8- 782 J-Ks=0.995+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:28.88 +59:54:38.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:28.88 +59:54:38.2: 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 04 28.4429* 01 19 28.88 +59 54 38.2 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 510323036254643328,2461158.9429,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510323036254643328 20260428.4429 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.24 01:43:03.28 +58:57:14.2
129.55623 -3.25233 galactic Cas Second-epoch detections are separated by 0.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.7767+58.9545 | 01:43:03.28 +58:57:14.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.236+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:03.28 +58:57:14.2: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:03.28 +58:57:14.2: 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 04 28.4429* 01 43 03.28 +58 57 14.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.7767+58.9545,2461158.9429,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.7767+58.9545 20260428.4429 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 04 28.4429 2461158.9429 11.13 01:14:58.41 +60:30:23.9
125.82703 -2.23274 galactic Cas Second-epoch detections are separated by 2.5" and 6.6 pix
The object was found in VSX 3" Mis V1361
Type: EA
# Max. Min./Amp. JD0 Period
13.551 r Y 0.490 r 2458282.97450 1.603348400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:58.41 +60:30:23.9: 12.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:58.41 +60:30:23.9: 13.65 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 04 28.4429* 01 14 58.41 +60 30 23.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1361,2461158.9429,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V1361 20260428.4429 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.29 02:01:03.69 +64:43:34.2
130.27869 2.85218 galactic Cas Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:01:03.69 +64:43:34.2 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:03.69 +64:43:34.2: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:03.69 +64:43:34.2: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 02 01 03.69 +64 43 34.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,11.29,0.05,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
target 20260428.4429 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 04 28.4429 2461158.9429 11.30 01:48:34.97 +58:41:32.3
130.31187 -3.35823 galactic Cas Second-epoch detections are separated by 5.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J027.1136+58.6801 | 01:48:31.31 +58:41:04.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:34.97 +58:41:32.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:34.97 +58:41:32.3: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 48 34.97 +58 41 32.3 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
ATO J027.1136+58.6801,2461158.9429,11.30,0.05,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
ATO J027.1136+58.6801 20260428.4429 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 04 28.4429 2461158.9429 11.29 01:23:53.36 +60:53:22.7
126.87049 -1.73371 galactic Cas Second-epoch detections are separated by 3.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:23:53.36 +60:53:22.7 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.164 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:53.36 +60:53:22.7: 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 01:23:53.36 +60:53:22.7: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 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 04 28.4429* 01 23 53.36 +60 53 22.7 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
target,2461158.9429,11.29,0.05,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
target 20260428.4429 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 04 28.4429 2461158.9429 11.21 01:51:26.68 +57:51:35.7
130.86724 -4.08434 galactic Per Second-epoch detections are separated by 1.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506162862211871616 | 01:51:29.54 +57:50:59.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.266+/-0.053 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:26.68 +57:51:35.7: 13.12 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:26.68 +57:51:35.7: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 04 28.4429* 01 51 26.68 +57 51 35.7 11.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506162862211871616,2461158.9429,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506162862211871616 20260428.4429 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4429 2461158.9429 11.32 01:59:34.05 +63:37:07.7
130.41383 1.74110 galactic Cas Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:34.05 +63:37:07.7 (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 01:59:34.05 +63:37:07.7: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:34.05 +63:37:07.7: 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 04 28.4429* 01 59 34.05 +63 37 07.7 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
target,2461158.9429,11.32,0.05,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
target 20260428.4429 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 04 28.4429 2461158.9429 11.44 01:52:55.27 +59:33:30.5
130.65667 -2.38799 galactic Cas Second-epoch detections are separated by 2.9" and 6.8 pix
The object was found in VSX17" Gaia DR3 506553498077188608
Type: ROT
# Max. Min./Amp. JD0 Period
15.360 G 15.380 G 2.474540000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:55.27 +59:33:30.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:55.27 +59:33:30.5: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 52 55.27 +59 33 30.5 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 506553498077188608,2461158.9429,11.44,0.05,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 506553498077188608 20260428.4429 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 04 28.4429 2461158.9429 11.34 01:27:56.50 +62:46:06.7
127.09387 0.19213 galactic Cas Second-epoch detections are separated by 3.0" and 5.9 pix
The object was found in VSX 4" Gaia DR3 512378916841008256
Type: E
# Max. Min./Amp. JD0 Period
14.550 G 14.640 G 1.395540000000 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 01:27:56.50 +62:46:06.7: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:56.50 +62:46:06.7: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 04 28.4429* 01 27 56.50 +62 46 06.7 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 512378916841008256,2461158.9429,11.34,0.05,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
Gaia DR3 512378916841008256 20260428.4429 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 04 28.4429 2461158.9429 11.43 01:31:48.45 +64:22:28.8
127.28061 1.84431 galactic Cas Second-epoch detections are separated by 4.1" and 5.4 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 | 01:31:48.45 +64:22:28.8 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.45 +64:22:28.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.45 +64:22:28.8: 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 04 28.4429* 01 31 48.45 +64 22 28.8 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,2461158.9429,11.43,0.05,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 20260428.4429 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 04 28.4429 2461158.9429 11.33 02:00:33.04 +59:40:08.2
131.56374 -2.03953 galactic Cas Second-epoch detections are separated by 1.2" and 6.4 pix
The object was found in VSX 1" ZTF J020033.07+594008.7
Type: SR
# Max. Min./Amp. JD0 Period
13.621 r Y 0.477 r 2458342.93970 344.838134100000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:33.04 +59:40:08.2: 11.84 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:33.04 +59:40:08.2: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 04 28.4429* 02 00 33.04 +59 40 08.2 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
ZTF J020033.07+594008.7,2461158.9429,11.33,0.05,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
ZTF J020033.07+594008.7 20260428.4429 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 04 28.4429 2461158.9429 11.46 01:42:17.67 +63:24:21.8
128.58720 1.09409 galactic Cas Second-epoch detections are separated by 0.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512081945620708864 | 01:42:22.23 +63:24:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.949+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:17.67 +63:24:21.8: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:17.67 +63:24:21.8: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 42 17.67 +63 24 21.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512081945620708864,2461158.9429,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512081945620708864 20260428.4429 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 04 28.4429 2461158.9429 11.47 01:25:19.12 +59:52:41.5
127.17577 -2.71409 galactic Cas Second-epoch detections are separated by 2.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510097945609143168 | 01:25:17.72 +59:52:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.939+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:19.12 +59:52:41.5: 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 01:25:19.12 +59:52:41.5: 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 04 28.4429* 01 25 19.12 +59 52 41.5 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 510097945609143168,2461158.9429,11.47,0.05,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 510097945609143168 20260428.4429 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 04 28.4429 2461158.9429 11.69 01:38:40.38 +64:31:54.7
127.98393 2.12443 galactic Cas Second-epoch detections are separated by 2.0" and 6.2 pix
The object was found in VSX20" Gaia DR3 512964166264921856
Type: YSO
# Max. Min./Amp. JD0 Period
17.250 G 17.380 G M
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 01:38:40.38 +64:31:54.7: 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 01:38:40.38 +64:31:54.7: 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 04 28.4429* 01 38 40.38 +64 31 54.7 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 512964166264921856,2461158.9429,11.69,0.05,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
Gaia DR3 512964166264921856 20260428.4429 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 04 28.4429 2461158.9429 11.56 01:58:46.65 +60:45:03.3
131.06841 -1.05262 galactic Cas Second-epoch detections are separated by 0.2" and 6.1 pix
The object was found in VSX24" Gaia DR3 508026740578798208
Type: ROT
# Max. Min./Amp. JD0 Period
15.330 G 15.370 G M
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 01:58:46.65 +60:45:03.3: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:46.65 +60:45:03.3: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 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 04 28.4429* 01 58 46.65 +60 45 03.3 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 508026740578798208,2461158.9429,11.56,0.05,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 508026740578798208 20260428.4429 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 04 28.4429 2461158.9429 11.60 01:35:35.66 +61:15:46.7
128.21519 -1.15500 galactic Cas Second-epoch detections are separated by 1.7" and 6.6 pix
The object was found in VSX 1" Gaia DR3 509978133204810624
Type: RS
# Max. Min./Amp. JD0 Period
14.210 G 14.320 G 2.136390000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:35.66 +61:15:46.7: 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 01:35:35.66 +61:15:46.7: 14.22 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 35 35.66 +61 15 46.7 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 509978133204810624,2461158.9429,11.60,0.05,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
Gaia DR3 509978133204810624 20260428.4429 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 04 28.4429 2461158.9429 10.99 01:33:44.60 +60:46:16.7
128.07615 -1.67720 galactic Cas Second-epoch detections are separated by 5.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:44.60 +60:46:16.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:44.60 +60:46:16.7: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.60 +60:46:16.7: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.4429* 01 33 44.60 +60 46 16.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.9429,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.4429 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461158.94324185 28.04.2026 10:38:06.096 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 25251
Objects passed selection criteria: 25092
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 17172.2
Average stars matched: 15797.2 (91.9929 %)
Memory usage VmPeak: 128284 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 28 05:56:14 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461158.94324185 28.04.2026 10:38:06.096 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 210
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 75 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 184909
Objects passed selection criteria: 184405
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 134777
Average stars matched: 123930 (91.9519 %)
Memory usage VmPeak: 2000196 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 28 06:01:36 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461158.94264932
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_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits'
wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.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_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:33.187 +62:01:47.22 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 01:42:33.187 +62:01:47.22
Angular distance between the image centers 0.0455 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:30.153 +62:02:17.31 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 01:42:30.153 +62:02:17.31
Angular distance between the image centers 0.0531 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 01:42:33.187 +62:01:47.22
Second-epoch second image center 01:42:30.153 +62:02:17.31
Angular distance between the image centers 0.01025 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.3CiAAwIFH7
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.Hj5vWPIUkT
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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits &> /tmp/tmp.FtvqV5UkvY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits &> /tmp/tmp.qGIeR4fdka
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.729996
a=0.000000 b=1.000000 c=22.729996
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.11
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.11
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
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
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.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:
15.1 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.1 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
14.0 mag. fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
14.0 mag. fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.3CiAAwIFH7 (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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 266 matched stars entering correct_measured_positions(), 9996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 337 matched stars entering correct_measured_positions(), 10041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.88"
Excluding outliers - 331 stars left (next iteration limit 292)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Hj5vWPIUkT (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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FtvqV5UkvY (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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.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_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=991, passed=13608
Got 13608 stars (including 12602 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat
util/solve_plate_with_UCAC5 got 13608 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 13350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 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
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 13350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 13350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 970 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits -region wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qGIeR4fdka (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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.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_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=997, passed=13538
Got 13538 stars (including 12534 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat
util/solve_plate_with_UCAC5 got 13538 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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: 971 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 13306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 13306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 13306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 970 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits -region wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53357.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51603_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 51603_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:09:11.30 +58:01:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 0.577 506734299021796736 032.29686537894 +58.01777790372 10.9407 10.6614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52692_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 52692_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:19:46.46 +58:12:25.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53357_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 53357_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:33:24.40 +60:39:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.75, MAG_FAINT_SEARCH_LIMIT=11.73)GAIADR2_OUTPUT=# 0.825 509862924996841984 023.35139623571 +60.66242410040 11.2048 10.9125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 08339_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:20:32.56 +62:32:00.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
Image size: 938.9'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:33.187 +62:01:47.22 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 01:42:33.187 +62:01:47.22
Angular distance between the image centers 0.0455 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:30.153 +62:02:17.31 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 01:42:30.153 +62:02:17.31
Angular distance between the image centers 0.0531 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 01:42:33.187 +62:01:47.22
Second-epoch second image center 01:42:30.153 +62:02:17.31
Angular distance between the image centers 0.01025 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.4Puky8QkYh
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.Z4676kKAmS
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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits &> /tmp/tmp.TC8b1dMEsg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits &> /tmp/tmp.cnj6wSH0OQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.332900
a=0.000000 b=1.000000 c=20.332900
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.05
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.05
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=4.4)
Read 218998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9707 to 45.8168 deg, Dec +55.3262 to +67.4140 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9707 to 45.8168 deg, Dec 55.3262 to 67.4140 deg
Loaded 26295 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10859 out of 16691 total matches.
Matched with Tycho-2 16691 out of 218998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 192 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.2 pix fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
2.2 pix fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
13.1 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
13.0 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
11.9 mag. fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
11.9 mag. fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
All-image limiting magnitude estimate: 11.9 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.4Puky8QkYh (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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=35398, passed=222522
Got 222522 stars (including 186791 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 222522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 275 matched stars entering correct_measured_positions(), 212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 264 matched stars entering correct_measured_positions(), 49591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 434 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 49636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
Accuracy estimation diagnostic: 344 matched stars entering correct_measured_positions(), 64908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.78"
Excluding outliers - 344 stars left (next iteration limit 290)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Z4676kKAmS (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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=35098, passed=218974
Got 218974 stars (including 183551 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 218974 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TC8b1dMEsg (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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.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_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=9399, passed=105767
Got 105767 stars (including 96240 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat
util/solve_plate_with_UCAC5 got 105767 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 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: 970 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 104223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 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
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 104223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 104224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 969 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits -region wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cnj6wSH0OQ (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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.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_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.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_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=9330, passed=106245
Got 106245 stars (including 96803 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat
util/solve_plate_with_UCAC5 got 106245 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 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: 970 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 104866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 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
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 104867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 104868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 969 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits -region wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-37-14_20.00sec_-4.90C_LIGHT_0300.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Cas-03-Q2b1x1_054905_TTUQ2b1x1_3006143_EOwzxFKY/wcs_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301.fits
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out125111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271492.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 135s
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: 55s
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Considering the candidate 247624_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247624_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247638_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247638_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247642_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247642_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247645_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247645_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247649_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247649_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247650_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247650_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247658_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247658_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247659_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247659_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247669_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247669_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247670_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247670_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247671_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247671_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247673_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247673_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247682_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247682_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:49:01.03 +60:33:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247688_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247688_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247694_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247694_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247701_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247701_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247706_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247706_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247711_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247711_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247712_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247712_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247714_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247714_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247715_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247715_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247719_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247719_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247721_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247721_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247722_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247722_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247723_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247723_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247724_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247724_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247726_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247726_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:41.21 +65:22:37.8: 10.61 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:41.21 +65:22:37.8: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.02
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Considering the candidate 247727_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247727_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:39:24.14 +58:23:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247732_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247732_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247733_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247733_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247735_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247735_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 247736_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247736_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:29:22.22 +63:18:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247738_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247738_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247745_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247745_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:33:35.29 +59:56:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247746_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247746_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247750_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247750_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:10.40 +60:37:29.8: 7.83 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:10.40 +60:37:29.8: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 8.06 +/- 0.01
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Considering the candidate 247751_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247751_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:32:22.11 +60:27:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247753_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247753_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:53.85 +59:29:53.8: 9.92 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:53.85 +59:29:53.8: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.63 +/- 0.01
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Considering the candidate 247755_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247755_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247758_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247758_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247763_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247763_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:07:34.08 +60:52:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247764_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247764_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247767_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247767_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:46:42.47 +61:09:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247770_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247770_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247771_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247771_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247787_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247787_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247790_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247790_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247791_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247791_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247794_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247794_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:07:07.96 +57:44:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247795_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247795_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247796_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247796_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247797_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247797_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247798_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247798_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247799_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 247799_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:43:59.15 +61:55:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247800_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247800_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247803_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247803_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247806_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247806_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247809_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247809_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247810_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247810_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 247811_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 247811_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 251931_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 251931_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:46:08.63 +61:12:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252023_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 252023_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:44:02.23 +61:53:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252431_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 252431_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 252791_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 252791_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:38:00.49 +57:56:46.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253448_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 253448_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:17:59.19 +57:47:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254927_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 254927_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 255567_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 255567_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:19:12.21 +65:35:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255789_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 255789_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:28:15.38 +58:44:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255935_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 255935_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 256859_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 256859_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:20:10.91 +58:12:10.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 257094_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 257094_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:58:16.37 +59:38:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257676_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 257676_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:16:08.53 +58:49:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257875_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 257875_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:51:02.37 +64:49:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257921_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 257921_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:44:17.69 +61:53:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257922_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 257922_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 258001_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 258001_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:43:53.12 +61:53:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258113_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 258113_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:46:33.59 +61:16:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258603_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 258603_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:33:59.42 +58:28:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258839_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 258839_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 259118_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 259118_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:15:58.83 +63:12:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259607_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 259607_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:43:03.22 +58:08:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259859_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 259859_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 259863_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 259863_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:02:54.94 +64:24:57.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259890_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 259890_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 259969_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 259969_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 260133_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 260133_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:00:51.81 +58:31:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260286_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 260286_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:19:22.28 +58:19:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260296_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 260296_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:13:35.93 +57:52:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260381_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 260381_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:00.98 +60:12:40.0: 9.78 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:00.98 +60:12:40.0: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.42 +/- 0.01
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Considering the candidate 260691_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 260691_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:00:36.75 +58:30:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260696_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 260696_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:34:10.33 +62:09:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260814_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 260814_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:27:02.20 +58:03:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261184_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 261184_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:44:01.42 +61:52:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261219_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 261219_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 261435_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 261435_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:39:56.89 +60:52:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261704_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 261704_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:48:38.18 +61:49:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261727_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 261727_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:16:05.01 +58:49:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261886_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 261886_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:37:44.74 +64:45:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261954_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 261954_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:42:32.99 +63:52:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262046_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 262046_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:38:08.32 +61:03:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262130_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 262130_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:04:26.77 +65:05:52.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262201_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 262201_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 262254_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 262254_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:15:11.35 +60:07:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262491_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 262491_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:33:23.22 +57:44:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262599_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 262599_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:35:54.14 +60:13:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262631_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 262631_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:47:18.74 +63:38:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262703_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 262703_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:26:41.00 +60:46:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262767_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 262767_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 262871_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 262871_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:13:30.58 +58:34:23.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263024_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 263024_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:58:40.27 +59:15:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263035_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 263035_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:41:50.97 +61:02:07.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263069_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 263069_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:06:23.43 +62:44:02.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263077_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 263077_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 263511_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 263511_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:37:13.64 +58:38:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263563_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 263563_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:35:50.55 +61:27:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263666_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 263666_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 263687_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 263687_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 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 263712_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 263712_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:01:15.08 +59:23:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263934_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 263934_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:19:03.89 +63:57:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263938_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 263938_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:44:27.71 +60:41:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264084_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264084_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:54:18.90 +63:38:04.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 264158_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 264158_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 264207_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 264207_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 264245_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 264245_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 264272_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264272_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:16:36.69 +64:56:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264320_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264320_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:49:34.26 +61:03:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264335_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264335_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:44:56.72 +59:46:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264371_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264371_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:06:45.46 +59:50:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264430_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264430_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:38:33.81 +60:47:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264512_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264512_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:55:53.08 +64:15:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264698_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264698_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:01:36.92 +59:57:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264772_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264772_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:03:15.34 +62:12:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264840_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 264840_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:23:07.59 +61:11:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265121_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 265121_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:18:04.29 +65:36:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265125_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 265125_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:31:32.59 +61:02:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265129_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 265129_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:43:07.14 +58:57:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265132_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 265132_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:01:38.85 +61:45:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265267_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 265267_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 265528_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 265528_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:38:07.66 +61:01:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265591_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 265591_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:02:53.94 +60:15:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265617_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 265617_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:14:30.03 +63:16:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265671_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 265671_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 265749_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 265749_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:10:32.35 +59:59:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265903_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 265903_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 265931_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 265931_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:42:54.76 +64:01:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266090_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 266090_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 266101_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266101_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:34:42.57 +58:42:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266175_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266175_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:20:40.70 +60:23:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266192_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266192_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:46:50.78 +60:39:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266223_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 266223_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 266306_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266306_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:48:39.88 +59:09:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266327_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 266327_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 266335_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266335_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:36.33 +60:53:50.4: 10.09 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:36.33 +60:53:50.4: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.03
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Considering the candidate 266429_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266429_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:37:12.98 +58:38:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266447_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266447_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:38:11.99 +61:01:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266634_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266634_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:43:12.89 +64:00:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266769_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266769_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:07:03.88 +59:51:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266864_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 266864_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 266877_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266877_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:17:21.65 +59:22:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266929_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 266929_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:38:06.56 +58:10:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266969_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 266969_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 267032_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 267032_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:14:00.82 +59:02:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267086_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 267086_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 267195_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 267195_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:37:41.56 +58:37:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267235_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 267235_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 267509_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 267509_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 267691_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 267691_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 267758_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 267758_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:15:05.64 +64:08:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267887_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 267887_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 268060_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 268060_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 268115_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 268115_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 268297_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 268297_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:55:21.48 +59:25:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268442_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 268442_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 268981_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 268981_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 269208_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 269208_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 269433_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 269433_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:44:32.18 +61:36:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269444_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 269444_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 269980_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 269980_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 270209_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 270209_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:42:26.68 +59:34:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270471_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 270471_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:49:05.99 +65:23:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270497_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 270497_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 270578_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 270578_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 270740_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 270740_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 270829_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 270829_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 271408_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 271408_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 271440_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 271440_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 271492_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 271492_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 39378_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:47:55.65 +64:32:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 72532_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:45:35.70 +63:07:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125111_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
Preparing report for the candidate 125111_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
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Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 70271_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:20:32.53 +62:32:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301
The candidate 76113_fd_Cas-03-Q2b1x1_2026-04-28_05-38-06_20.00sec_-5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:02:02.20 +62:41:31.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 194s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:33:44.60 +60:46:16.7
01:43:20.59 +61:14:37.2
01:22:33.09 +60:44:41.8
01:12:30.20 +62:02:37.7
02:00:50.08 +62:37:50.5
01:55:46.55 +57:57:43.0
01:59:11.69 +65:05:59.3
01:47:51.34 +61:11:12.6
01:13:01.23 +61:00:59.2
01:37:23.70 +59:20:12.8
01:23:56.46 +62:15:25.4
01:12:41.33 +61:18:07.0
01:10:12.01 +59:17:25.2
02:00:06.54 +59:00:31.6
01:24:54.87 +59:41:46.2
01:08:39.00 +60:32:41.9
01:12:09.70 +58:47:54.0
01:14:01.30 +57:40:45.9
01:07:39.25 +59:59:18.1
01:33:01.59 +59:16:33.9
01:43:27.28 +59:35:12.7
01:43:27.30 +58:38:07.8
01:26:05.48 +59:01:14.5
01:56:43.16 +58:07:16.3
01:07:34.94 +57:33:09.7
01:07:41.68 +60:54:05.7
01:10:43.79 +60:59:19.6
01:15:23.08 +61:11:40.9
01:42:44.41 +58:39:00.7
01:49:15.97 +59:14:38.1
01:19:23.99 +58:26:39.7
01:31:22.92 +59:33:42.3
01:25:15.25 +64:40:33.2
02:13:47.56 +58:44:00.0
01:09:46.02 +58:12:06.5
01:14:45.34 +60:30:04.0
01:12:40.98 +61:20:38.9
01:07:57.19 +63:37:32.5
01:15:55.97 +58:23:29.5
01:55:14.56 +59:32:02.5
01:35:24.92 +60:39:14.9
01:57:04.02 +64:41:41.6
01:15:16.84 +57:28:04.4
01:20:24.41 +59:10:24.7
01:19:48.74 +61:38:15.1
01:25:56.60 +59:35:11.9
01:16:00.98 +62:41:57.8
02:13:07.47 +58:04:48.1
01:19:11.07 +58:20:31.4
01:25:42.74 +65:40:08.9
01:18:14.21 +61:44:36.6
02:15:40.50 +62:14:22.0
02:06:39.03 +64:09:28.7
02:20:52.98 +63:53:40.1
01:44:32.31 +58:45:36.4
02:11:23.05 +61:21:06.1
02:16:36.25 +64:57:46.7
01:39:24.65 +63:23:54.6
02:11:50.19 +59:02:57.3
01:19:41.51 +62:51:06.1
01:40:34.78 +60:45:54.2
01:46:38.46 +60:07:33.0
01:58:04.34 +57:58:50.4
01:44:46.18 +57:50:37.1
01:38:33.99 +58:07:23.8
02:02:41.62 +59:59:00.2
01:36:16.29 +60:12:24.4
02:10:23.84 +60:01:13.5
01:31:48.20 +64:21:56.8
01:32:05.68 +61:59:25.7
01:48:29.91 +60:27:35.3
01:50:39.66 +62:00:55.2
01:59:05.82 +59:55:35.2
01:19:28.88 +59:54:38.2
01:43:03.28 +58:57:14.2
01:14:58.41 +60:30:23.9
02:01:03.69 +64:43:34.2
01:48:34.97 +58:41:32.3
01:23:53.36 +60:53:22.7
01:51:26.68 +57:51:35.7
01:59:34.05 +63:37:07.7
01:52:55.27 +59:33:30.5
01:27:56.50 +62:46:06.7
01:31:48.45 +64:22:28.8
02:00:33.04 +59:40:08.2
01:42:17.67 +63:24:21.8
01:25:19.12 +59:52:41.5
01:38:40.38 +64:31:54.7
01:58:46.65 +60:45:03.3
01:35:35.66 +61:15:46.7
########### 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 ####
01:43:20.59 +61:14:37.2
01:22:33.09 +60:44:41.8
01:12:30.20 +62:02:37.7
02:00:50.08 +62:37:50.5
01:55:46.55 +57:57:43.0
01:59:11.69 +65:05:59.3
01:47:51.34 +61:11:12.6
01:13:01.23 +61:00:59.2
01:37:23.70 +59:20:12.8
01:23:56.46 +62:15:25.4
01:12:41.33 +61:18:07.0
01:10:12.01 +59:17:25.2
02:00:06.54 +59:00:31.6
01:24:54.87 +59:41:46.2
01:08:39.00 +60:32:41.9
01:12:09.70 +58:47:54.0
01:14:01.30 +57:40:45.9
01:07:39.25 +59:59:18.1
01:33:01.59 +59:16:33.9
01:43:27.28 +59:35:12.7
01:43:27.30 +58:38:07.8
01:26:05.48 +59:01:14.5
01:56:43.16 +58:07:16.3
01:07:34.94 +57:33:09.7
01:07:41.68 +60:54:05.7
01:10:43.79 +60:59:19.6
01:15:23.08 +61:11:40.9
01:42:44.41 +58:39:00.7
01:49:15.97 +59:14:38.1
01:19:23.99 +58:26:39.7
01:31:22.92 +59:33:42.3
01:25:15.25 +64:40:33.2
02:13:47.56 +58:44:00.0
01:09:46.02 +58:12:06.5
01:14:45.34 +60:30:04.0
01:12:40.98 +61:20:38.9
01:07:57.19 +63:37:32.5
01:15:55.97 +58:23:29.5
01:55:14.56 +59:32:02.5
01:35:24.92 +60:39:14.9
01:57:04.02 +64:41:41.6
01:15:16.84 +57:28:04.4
01:20:24.41 +59:10:24.7
01:19:48.74 +61:38:15.1
01:25:56.60 +59:35:11.9
01:16:00.98 +62:41:57.8
02:13:07.47 +58:04:48.1
01:19:11.07 +58:20:31.4
01:25:42.74 +65:40:08.9
01:18:14.21 +61:44:36.6
02:15:40.50 +62:14:22.0
02:06:39.03 +64:09:28.7
02:20:52.98 +63:53:40.1
01:44:32.31 +58:45:36.4
02:11:23.05 +61:21:06.1
02:16:36.25 +64:57:46.7
01:39:24.65 +63:23:54.6
02:11:50.19 +59:02:57.3
01:19:41.51 +62:51:06.1
01:40:34.78 +60:45:54.2
01:46:38.46 +60:07:33.0
01:58:04.34 +57:58:50.4
01:44:46.18 +57:50:37.1
01:38:33.99 +58:07:23.8
02:02:41.62 +59:59:00.2
01:36:16.29 +60:12:24.4
02:10:23.84 +60:01:13.5
01:31:48.20 +64:21:56.8
01:32:05.68 +61:59:25.7
01:48:29.91 +60:27:35.3
01:50:39.66 +62:00:55.2
01:59:05.82 +59:55:35.2
01:19:28.88 +59:54:38.2
01:43:03.28 +58:57:14.2
01:14:58.41 +60:30:23.9
02:01:03.69 +64:43:34.2
01:48:34.97 +58:41:32.3
01:23:53.36 +60:53:22.7
01:51:26.68 +57:51:35.7
01:59:34.05 +63:37:07.7
01:52:55.27 +59:33:30.5
01:27:56.50 +62:46:06.7
01:31:48.45 +64:22:28.8
02:00:33.04 +59:40:08.2
01:42:17.67 +63:24:21.8
01:25:19.12 +59:52:41.5
01:38:40.38 +64:31:54.7
01:58:46.65 +60:45:03.3
01:35:35.66 +61:15:46.7
01:33:44.60 +60:46:16.7
###################################################################################
01:43:20.59 +61:14:37.2 -- not an asteroid (will add it to exclusion list)
01:22:33.09 +60:44:41.8 -- not an asteroid (will add it to exclusion list)
01:12:30.20 +62:02:37.7 -- not an asteroid (will add it to exclusion list)
02:00:50.08 +62:37:50.5 -- not an asteroid (will add it to exclusion list)
01:55:46.55 +57:57:43.0 -- not an asteroid (will add it to exclusion list)
01:59:11.69 +65:05:59.3 -- not an asteroid (will add it to exclusion list)
01:47:51.34 +61:11:12.6 -- not an asteroid (will add it to exclusion list)
01:13:01.23 +61:00:59.2 -- not an asteroid (will add it to exclusion list)
01:37:23.70 +59:20:12.8 -- not an asteroid (will add it to exclusion list)
01:23:56.46 +62:15:25.4 -- not an asteroid (will add it to exclusion list)
01:12:41.33 +61:18:07.0 -- not an asteroid (will add it to exclusion list)
01:10:12.01 +59:17:25.2 -- not an asteroid (will add it to exclusion list)
02:00:06.54 +59:00:31.6 -- not an asteroid (will add it to exclusion list)
01:24:54.87 +59:41:46.2 -- not an asteroid (will add it to exclusion list)
01:08:39.00 +60:32:41.9 -- not an asteroid (will add it to exclusion list)
01:12:09.70 +58:47:54.0 -- not an asteroid (will add it to exclusion list)
01:14:01.30 +57:40:45.9 -- not an asteroid (will add it to exclusion list)
01:07:39.25 +59:59:18.1 -- not an asteroid (will add it to exclusion list)
01:33:01.59 +59:16:33.9 -- not an asteroid (will add it to exclusion list)
01:43:27.28 +59:35:12.7 -- not an asteroid (will add it to exclusion list)
01:43:27.30 +58:38:07.8 -- not an asteroid (will add it to exclusion list)
01:26:05.48 +59:01:14.5 -- not an asteroid (will add it to exclusion list)
01:56:43.16 +58:07:16.3 -- not an asteroid (will add it to exclusion list)
01:07:34.94 +57:33:09.7 -- not an asteroid (will add it to exclusion list)
01:07:41.68 +60:54:05.7 -- not an asteroid (will add it to exclusion list)
01:10:43.79 +60:59:19.6 -- not an asteroid (will add it to exclusion list)
01:15:23.08 +61:11:40.9 -- not an asteroid (will add it to exclusion list)
01:42:44.41 +58:39:00.7 -- not an asteroid (will add it to exclusion list)
01:49:15.97 +59:14:38.1 -- not an asteroid (will add it to exclusion list)
01:19:23.99 +58:26:39.7 -- not an asteroid (will add it to exclusion list)
01:31:22.92 +59:33:42.3 -- not an asteroid (will add it to exclusion list)
01:25:15.25 +64:40:33.2 -- not an asteroid (will add it to exclusion list)
02:13:47.56 +58:44:00.0 -- not an asteroid (will add it to exclusion list)
01:09:46.02 +58:12:06.5 -- not an asteroid (will add it to exclusion list)
01:14:45.34 +60:30:04.0 -- not an asteroid (will add it to exclusion list)
01:12:40.98 +61:20:38.9 -- not an asteroid (will add it to exclusion list)
01:07:57.19 +63:37:32.5 -- not an asteroid (will add it to exclusion list)
01:15:55.97 +58:23:29.5 -- not an asteroid (will add it to exclusion list)
01:55:14.56 +59:32:02.5 -- not an asteroid (will add it to exclusion list)
01:35:24.92 +60:39:14.9 -- not an asteroid (will add it to exclusion list)
01:57:04.02 +64:41:41.6 -- not an asteroid (will add it to exclusion list)
01:15:16.84 +57:28:04.4 -- not an asteroid (will add it to exclusion list)
01:20:24.41 +59:10:24.7 -- not an asteroid (will add it to exclusion list)
01:19:48.74 +61:38:15.1 -- not an asteroid (will add it to exclusion list)
01:25:56.60 +59:35:11.9 -- not an asteroid (will add it to exclusion list)
01:16:00.98 +62:41:57.8 -- not an asteroid (will add it to exclusion list)
02:13:07.47 +58:04:48.1 -- not an asteroid (will add it to exclusion list)
01:19:11.07 +58:20:31.4 -- not an asteroid (will add it to exclusion list)
01:25:42.74 +65:40:08.9 -- not an asteroid (will add it to exclusion list)
01:18:14.21 +61:44:36.6 -- not an asteroid (will add it to exclusion list)
02:15:40.50 +62:14:22.0 -- not an asteroid (will add it to exclusion list)
02:06:39.03 +64:09:28.7 -- not an asteroid (will add it to exclusion list)
02:20:52.98 +63:53:40.1 -- not an asteroid (will add it to exclusion list)
01:44:32.31 +58:45:36.4 -- not an asteroid (will add it to exclusion list)
02:11:23.05 +61:21:06.1 -- not an asteroid (will add it to exclusion list)
02:16:36.25 +64:57:46.7 -- not an asteroid (will add it to exclusion list)
01:39:24.65 +63:23:54.6 -- not an asteroid (will add it to exclusion list)
02:11:50.19 +59:02:57.3 -- not an asteroid (will add it to exclusion list)
01:19:41.51 +62:51:06.1 -- not an asteroid (will add it to exclusion list)
01:40:34.78 +60:45:54.2 -- not an asteroid (will add it to exclusion list)
01:46:38.46 +60:07:33.0 -- not an asteroid (will add it to exclusion list)
01:58:04.34 +57:58:50.4 -- not an asteroid (will add it to exclusion list)
01:44:46.18 +57:50:37.1 -- not an asteroid (will add it to exclusion list)
01:38:33.99 +58:07:23.8 -- not an asteroid (will add it to exclusion list)
02:02:41.62 +59:59:00.2 -- not an asteroid (will add it to exclusion list)
01:36:16.29 +60:12:24.4 -- not an asteroid (will add it to exclusion list)
02:10:23.84 +60:01:13.5 -- not an asteroid (will add it to exclusion list)
01:31:48.20 +64:21:56.8 -- not an asteroid (will add it to exclusion list)
01:32:05.68 +61:59:25.7 -- not an asteroid (will add it to exclusion list)
01:48:29.91 +60:27:35.3 -- not an asteroid (will add it to exclusion list)
01:50:39.66 +62:00:55.2 -- not an asteroid (will add it to exclusion list)
01:59:05.82 +59:55:35.2 -- not an asteroid (will add it to exclusion list)
01:19:28.88 +59:54:38.2 -- not an asteroid (will add it to exclusion list)
01:43:03.28 +58:57:14.2 -- not an asteroid (will add it to exclusion list)
01:14:58.41 +60:30:23.9 -- not an asteroid (will add it to exclusion list)
02:01:03.69 +64:43:34.2 -- not an asteroid (will add it to exclusion list)
01:48:34.97 +58:41:32.3 -- not an asteroid (will add it to exclusion list)
01:23:53.36 +60:53:22.7 -- not an asteroid (will add it to exclusion list)
01:51:26.68 +57:51:35.7 -- not an asteroid (will add it to exclusion list)
01:59:34.05 +63:37:07.7 -- not an asteroid (will add it to exclusion list)
01:52:55.27 +59:33:30.5 -- not an asteroid (will add it to exclusion list)
01:27:56.50 +62:46:06.7 -- not an asteroid (will add it to exclusion list)
01:31:48.45 +64:22:28.8 -- not an asteroid (will add it to exclusion list)
02:00:33.04 +59:40:08.2 -- not an asteroid (will add it to exclusion list)
01:42:17.67 +63:24:21.8 -- not an asteroid (will add it to exclusion list)
01:25:19.12 +59:52:41.5 -- not an asteroid (will add it to exclusion list)
01:38:40.38 +64:31:54.7 -- not an asteroid (will add it to exclusion list)
01:58:46.65 +60:45:03.3 -- not an asteroid (will add it to exclusion list)
01:35:35.66 +61:15:46.7 -- not an asteroid (will add it to exclusion list)
01:33:44.60 +60:46:16.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:07:34.94 +57:33:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.25 +59:59:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:41.68 +60:54:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:57.19 +63:37:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:39.00 +60:32:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:46.02 +58:12:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:12.01 +59:17:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:43.79 +60:59:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:09.70 +58:47:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:30.20 +62:02:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:40.98 +61:20:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:41.33 +61:18:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:01.23 +61:00:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:01.30 +57:40:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:45.34 +60:30:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:58.41 +60:30:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:16.84 +57:28:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:23.08 +61:11:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:55.97 +58:23:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:00.98 +62:41:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:14.21 +61:44:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:11.07 +58:20:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:23.99 +58:26:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:28.88 +59:54:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:41.51 +62:51:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:48.74 +61:38:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:24.41 +59:10:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:33.09 +60:44:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:53.36 +60:53:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:56.46 +62:15:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:54.87 +59:41:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:15.25 +64:40:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:19.12 +59:52:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:42.74 +65:40:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:56.60 +59:35:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.48 +59:01:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:56.50 +62:46:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:22.92 +59:33:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.20 +64:21:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.45 +64:22:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:05.68 +61:59:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:01.59 +59:16:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:44.60 +60:46:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:24.92 +60:39:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:35.66 +61:15:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:16.29 +60:12:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:23.70 +59:20:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:33.99 +58:07:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:40.38 +64:31:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:24.65 +63:23:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:34.78 +60:45:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:17.67 +63:24:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:44.41 +58:39:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:03.28 +58:57:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:20.59 +61:14:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:27.28 +59:35:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:27.30 +58:38:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:32.31 +58:45:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:46.18 +57:50:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.46 +60:07:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:51.34 +61:11:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:29.91 +60:27:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:34.97 +58:41:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:15.97 +59:14:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:39.66 +62:00:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:26.68 +57:51:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:55.27 +59:33:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:14.56 +59:32:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:46.55 +57:57:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:43.16 +58:07:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:04.02 +64:41:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:04.34 +57:58:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:46.65 +60:45:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:05.82 +59:55:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:11.69 +65:05:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:34.05 +63:37:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:06.54 +59:00:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:33.04 +59:40:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:50.08 +62:37:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:03.69 +64:43:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:41.62 +59:59:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:39.03 +64:09:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:23.84 +60:01:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:23.05 +61:21:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:50.19 +59:02:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:07.47 +58:04:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:47.56 +58:44:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:40.50 +62:14:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:36.25 +64:57:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:52.98 +63:53:40.1 -- 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)
01:07:34.94 +57:33:09.7 -- not a known variable star
01:07:39.25 +59:59:18.1 -- not a known variable star
01:07:41.68 +60:54:05.7 -- not a known variable star
01:07:57.19 +63:37:32.5 -- a known variable star
01:08:39.00 +60:32:41.9 -- not a known variable star
01:09:46.02 +58:12:06.5 -- not a known variable star
01:10:12.01 +59:17:25.2 -- not a known variable star
01:10:43.79 +60:59:19.6 -- not a known variable star
01:12:09.70 +58:47:54.0 -- not a known variable star
01:12:30.20 +62:02:37.7 -- not a known variable star
01:12:40.98 +61:20:38.9 -- not a known variable star
01:12:41.33 +61:18:07.0 -- not a known variable star
01:13:01.23 +61:00:59.2 -- a known variable star
01:14:01.30 +57:40:45.9 -- not a known variable star
01:14:45.34 +60:30:04.0 -- not a known variable star
01:14:58.41 +60:30:23.9 -- a known variable star
01:15:16.84 +57:28:04.4 -- not a known variable star
01:15:23.08 +61:11:40.9 -- not a known variable star
01:15:55.97 +58:23:29.5 -- a known variable star
01:16:00.98 +62:41:57.8 -- not a known variable star
01:18:14.21 +61:44:36.6 -- not a known variable star
01:19:11.07 +58:20:31.4 -- not a known variable star
01:19:23.99 +58:26:39.7 -- not a known variable star
01:19:28.88 +59:54:38.2 -- not a known variable star
01:19:41.51 +62:51:06.1 -- not a known variable star
01:19:48.74 +61:38:15.1 -- not a known variable star
01:20:24.41 +59:10:24.7 -- not a known variable star
01:22:33.09 +60:44:41.8 -- not a known variable star
01:23:53.36 +60:53:22.7 -- not a known variable star
01:23:56.46 +62:15:25.4 -- not a known variable star
01:24:54.87 +59:41:46.2 -- not a known variable star
01:25:15.25 +64:40:33.2 -- not a known variable star
01:25:19.12 +59:52:41.5 -- not a known variable star
01:25:42.74 +65:40:08.9 -- not a known variable star
01:25:56.60 +59:35:11.9 -- not a known variable star
01:26:05.48 +59:01:14.5 -- not a known variable star
01:27:56.50 +62:46:06.7 -- a known variable star
01:31:22.92 +59:33:42.3 -- not a known variable star
01:31:48.20 +64:21:56.8 -- not a known variable star
01:31:48.45 +64:22:28.8 -- not a known variable star
01:32:05.68 +61:59:25.7 -- not a known variable star
01:33:01.59 +59:16:33.9 -- not a known variable star
01:33:44.60 +60:46:16.7 -- not a known variable star
01:35:24.92 +60:39:14.9 -- a known variable star
01:35:35.66 +61:15:46.7 -- a known variable star
01:36:16.29 +60:12:24.4 -- not a known variable star
01:37:23.70 +59:20:12.8 -- not a known variable star
01:38:33.99 +58:07:23.8 -- not a known variable star
01:38:40.38 +64:31:54.7 -- a known variable star
01:39:24.65 +63:23:54.6 -- not a known variable star
01:40:34.78 +60:45:54.2 -- not a known variable star
01:42:17.67 +63:24:21.8 -- not a known variable star
01:42:44.41 +58:39:00.7 -- not a known variable star
01:43:03.28 +58:57:14.2 -- not a known variable star
01:43:20.59 +61:14:37.2 -- not a known variable star
01:43:27.28 +59:35:12.7 -- not a known variable star
01:43:27.30 +58:38:07.8 -- a known variable star
01:44:32.31 +58:45:36.4 -- not a known variable star
01:44:46.18 +57:50:37.1 -- not a known variable star
01:46:38.46 +60:07:33.0 -- not a known variable star
01:47:51.34 +61:11:12.6 -- not a known variable star
01:48:29.91 +60:27:35.3 -- not a known variable star
01:48:34.97 +58:41:32.3 -- not a known variable star
01:49:15.97 +59:14:38.1 -- not a known variable star
01:50:39.66 +62:00:55.2 -- not a known variable star
01:51:26.68 +57:51:35.7 -- not a known variable star
01:52:55.27 +59:33:30.5 -- a known variable star
01:55:14.56 +59:32:02.5 -- not a known variable star
01:55:46.55 +57:57:43.0 -- a known variable star
01:56:43.16 +58:07:16.3 -- not a known variable star
01:57:04.02 +64:41:41.6 -- not a known variable star
01:58:04.34 +57:58:50.4 -- not a known variable star
01:58:46.65 +60:45:03.3 -- a known variable star
01:59:05.82 +59:55:35.2 -- not a known variable star
01:59:11.69 +65:05:59.3 -- not a known variable star
01:59:34.05 +63:37:07.7 -- not a known variable star
02:00:06.54 +59:00:31.6 -- not a known variable star
02:00:33.04 +59:40:08.2 -- a known variable star
02:00:50.08 +62:37:50.5 -- not a known variable star
02:01:03.69 +64:43:34.2 -- not a known variable star
02:02:41.62 +59:59:00.2 -- not a known variable star
02:06:39.03 +64:09:28.7 -- not a known variable star
02:10:23.84 +60:01:13.5 -- not a known variable star
02:11:23.05 +61:21:06.1 -- a known variable star
02:11:50.19 +59:02:57.3 -- a known variable star
02:13:07.47 +58:04:48.1 -- a known variable star
02:13:47.56 +58:44:00.0 -- not a known variable star
02:15:40.50 +62:14:22.0 -- not a known variable star
02:16:36.25 +64:57:46.7 -- not a known variable star
02:20:52.98 +63:53:40.1 -- not a known variable star
Found 74 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
90 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 90 (excluding asteroids and hot pixels, 74 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)2461158.94264932 -observatory V36
01:20:37.46 +06:08:47.9 Mercury (-0.6mag)
04:10:52.03 +21:52:00.6 Venus (-3.9mag)
00:53:06.51 +04:42:13.6 Mars (1.2mag)
07:19:03.93 +22:35:05.0 Jupiter (-2.0mag)
00:34:35.89 +01:22:23.5 Saturn (0.9mag)
03:50:26.30 +19:56:08.9 Uranus (5.8mag)
00:12:24.10 -00:05:36.5 Neptune (7.8mag)
20:34:08.83 -22:53:44.3 Pluto (14.5mag)
11:55:19.10 -02:32:32.6 Moon (-11.7mag)
-rw-r--r-- 1 apache apache 363 Apr 28 05:56 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461158.94264932:
07:19:03.74 +22:35:08.0 Io (5.8mag)
07:19:01.96 +22:35:07.0 Europa (6.0mag)
07:19:11.32 +22:34:54.8 Ganymede (5.4mag)
07:19:01.11 +22:35:20.2 Callisto (6.7mag)
07:21:47.32 +22:17:34.2 Himalia (15.4mag)
07:19:01.33 +22:35:12.7 Thebe (16.3mag)
07:22:11.48 +22:47:22.0 Elara (17.4mag)
07:18:47.21 +23:08:34.5 Pasiphae (17.5mag)
07:27:05.27 +22:34:09.5 Carme (18.6mag)
00:34:47.67 +01:22:26.8 Titan (8.8mag)
00:34:33.71 +01:22:39.2 Rhea (10.1mag)
00:34:06.24 +01:20:45.7 Iapetus (11.5mag)
00:34:40.41 +01:22:04.7 Hyperion (14.8mag)
00:36:02.13 +01:29:46.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 28 05:56 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461158.94264932:
16:23:17.53 -23:45:31.9 JWST
18:37:24.47 +24:40:51.6 Chandra
09:17:14.48 -53:01:51.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 28 05:56 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461158.94264932 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
06:10:09.14 +30:19:08.5 17.9mag P/2009 WX51 (Catalina)
18:55:26.24 -29:34:06.5 13.8mag P/2010 H2 (Vales)
05:16:17.11 -69:07:05.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:35:31.05 +31:31:54.5 17.3mag C/2017 K2 (PANSTARRS)
17:28:27.42 +11:58:11.5 17.7mag C/2021 G2 (ATLAS)
23:12:58.83 +29:45:35.7 17.1mag C/2022 E2 (ATLAS)
04:44:00.39 +26:21:16.5 16.1mag C/2022 N2 (PANSTARRS)
09:07:02.94 +32:00:16.5 16.3mag C/2022 QE78 (ATLAS)
08:33:42.81 +01:04:47.9 17.4mag C/2022 R6 (PANSTARRS)
18:49:56.57 +19:31:46.5 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:36:08.87 -11:20:21.5 17.5mag P/2023 B1 (PANSTARRS)
09:03:01.66 -10:00:08.2 17.8mag C/2023 F3 (ATLAS)
22:05:00.36 +63:41:39.8 17.6mag C/2023 H5 (Lemmon)
19:05:53.98 -04:01:42.0 14.0mag C/2023 R1 (PANSTARRS)
20:27:02.01 +87:37:29.0 17.8mag C/2023 X2 (Lemmon)
06:25:36.57 +63:30:52.6 17.3mag C/2024 A1 (ATLAS)
05:38:23.36 +21:46:57.3 11.8mag C/2024 E1 (Wierzchos)
16:10:31.16 +08:23:18.8 17.3mag C/2024 G6 (ATLAS)
20:23:13.97 +18:46:33.7 14.4mag C/2024 J3 (ATLAS)
03:37:51.69 -20:34:49.4 16.3mag C/2024 T5 (ATLAS)
05:27:41.61 +42:22:43.5 17.8mag C/2025 J1 (Borisov)
12:50:16.07 +51:03:05.9 15.8mag C/2025 L1 (ATLAS)
03:46:03.71 -28:18:12.3 17.9mag C/2025 Q3 (ATLAS)
03:07:53.55 +04:24:22.0 8.0mag C/2025 R3 (PANSTARRS)
12:48:57.81 +03:42:07.7 17.3mag C/2025 Y1 (ATLAS)
04:41:27.54 +01:49:21.2 16.0mag C/2026 A1 (MAPS)
00:33:07.28 +39:14:37.5 15.0mag C/2026 B2 (Sun-Gao)
19:07:01.39 -09:02:32.6 11.1mag 10P/Tempel
14:43:34.70 +01:42:03.8 15.1mag 24P/Schaumasse
11:00:11.91 -01:10:43.7 15.8mag 29P/Schwassmann-Wachmann
10:38:43.24 -03:16:04.8 17.2mag 43P/Wolf-Harrington
02:08:01.80 +19:33:48.4 17.3mag 47P/Ashbrook-Jackson
07:34:43.66 +34:14:57.3 17.0mag 63P/Wild
23:44:26.14 -10:00:57.2 15.7mag 65P/Gunn
04:37:41.09 +25:13:34.0 16.0mag 76P/West-Kohoutek-Ikemura
01:33:27.25 +10:37:22.3 14.2mag 78P/Gehrels
23:39:17.45 -05:43:39.2 14.8mag 88P/Howell
02:46:35.52 +23:45:54.1 15.0mag 93P/Lovas
05:19:19.62 +32:51:43.0 16.1mag 123P/West-Hartley
08:44:37.88 +32:39:08.0 16.3mag 124P/Mrkos
02:52:43.35 +15:42:39.8 16.4mag 128P/Shoemaker-Holt
03:12:07.29 +15:55:00.3 17.6mag 131P/Mueller
02:33:03.98 +16:53:42.2 10.6mag 141P/Machholz
02:39:48.43 +09:22:33.1 10.6mag 141P-A/Machholz
01:20:40.64 +05:06:47.8 11.5mag 141P-D/Machholz
01:37:27.49 +04:45:43.9 14.9mag 162P/SidingSpring
22:12:06.15 -08:31:38.2 17.9mag 218P/LINEAR
17:16:56.27 -12:24:16.3 16.1mag 235P/LINEAR
06:01:54.71 +35:27:07.0 16.9mag 240P/NEAT
07:45:30.67 -03:56:19.7 17.8mag 242P/Spahr
22:48:05.74 -17:25:16.8 17.5mag 260P/McNaught
02:24:28.59 +23:32:49.9 17.9mag 295P/LINEAR
15:36:59.72 +07:42:46.3 17.4mag 391P/Kowalski
07:39:49.54 +21:21:31.4 17.7mag 450P/LONEOS
05:54:35.17 +44:18:15.9 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 28 05:56 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
16:34:34.94 -54:34:58.20 2026-04-25.14 15.99
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
16:34:34.94 -54:34:58.20 2026-04-25.14 15.99
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
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
-rw-r--r-- 1 apache apache 5.8K Apr 28 05:56 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
-rw-r--r-- 1 apache apache 188K Apr 28 05:56 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:42:32.980 +27:19:40.88 AT 2026kgh 2026-04-10.49 20.4326
13:44:15.771 +09:32:24.71 AT 2026kgg 2026-04-16.32 19.297
12:32:26.606 -03:00:41.63 AT 2026kgf 2026-04-17.36 19.825
19:39:55.877 +11:06:48.06 AT 2026kge 2026-04-20.47 17.647
16:23:58.302 -04:09:47.64 AT 2026kgd 2026-04-18.46 16.784
19:23:59.111 -12:30:36.58 AT 2026kgc 2026-04-15.48 18.635
18:39:37.719 +06:55:20.96 AT 2026kgb 2026-04-17.43 16.308
15:06:42.954 -01:17:07.82 AT 2026kga 2026-04-20.40 19.507
17:53:09.200 +11:02:30.70 AT 2026kfz 2026-04-16.84 18.68
16:03:08.437 +31:48:52.12 AT 2026kfy 2026-04-15.37 20.9066
12:40:00.450 -17:44:25.00 AT 2026kfx 2026-04-21.19 17.9
09:56:52.772 +01:49:59.18 AT 2026kfw 2026-04-21.04 22.5328
09:59:02.400 +01:44:31.96 AT 2026kfv 2026-04-16.08 23.04
13:20:14.744 +79:52:47.47 AT 2026kfu 2026-04-20.39 20.1588
15:56:36.952 +46:26:50.20 AT 2026kft 2026-04-15.37 20.5825
14:36:13.311 -40:29:09.08 AT 2026kfs 2026-04-17.20 19.109
17:55:24.804 -72:52:42.49 AT 2026kfr 2026-04-19.04 19.559
14:53:17.557 +07:16:56.07 AT 2026kfq 2026-04-20.44 20.1681
14:23:33.083 +17:33:13.27 AT 2026kfp 2026-04-15.41 20.3946
11:23:12.007 -46:35:10.13 AT 2026kfo 2026-04-18.14 19.338
-rw-r--r-- 1 apache apache 29K Apr 28 05:56 tns_transients_list.txt
