This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.69 23:51:09.70 +53:46:57.8
114.00722 -8.04129 galactic Cas Second-epoch detections are separated by 1.7" and 7.4 pix
The object was found in VSX 3" Gaia DR3 1993473306253508480
Type: ROT
# Max. Min./Amp. JD0 Period
14.870 G 14.910 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:09.70 +53:46:57.8: 13.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:09.70 +53:46:57.8: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 51 09.70 +53 46 57.8 12.7 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 1993473306253508480,2461235.6690,12.69,0.05,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 1993473306253508480 20260714.1690 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.52 23:56:12.73 +54:27:13.9
114.88690 -7.55298 galactic Cas Second-epoch detections are separated by 0.8" and 7.1 pix
The object was found in VSX19" Gaia DR3 1993633074736513920
Type:
# Max. Min./Amp. JD0 Period
16.540 G 16.600 G K
ATTENTION: measured mag 12.52 is 4.0 mag brighter than the VSX record maximum brightness 16.54 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:56:12.73 +54:27:13.9: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:56:12.73 +54:27:13.9: 13.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 56 12.73 +54 27 13.9 12.5 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 1993633074736513920,2461235.6690,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993633074736513920 20260714.1690 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.55 23:58:03.04 +56:41:42.7
115.61695 -5.41641 galactic Cas Second-epoch detections are separated by 1.4" and 7.3 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 J359.5132+56.6947 | 23:58:03.04 +56:41:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.372+/-0.041 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:03.04 +56:41:42.7: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:03.04 +56:41:42.7: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 58 03.04 +56 41 42.7 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.5132+56.6947,2461235.6690,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.5132+56.6947 20260714.1690 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.53 00:21:25.15 +52:13:59.1
118.26759 -10.36659 galactic Cas Second-epoch detections are separated by 2.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:25.15 +52:13:59.1 (user input) | T | P | (position from user input) J-Ks=0.653+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:21:25.15 +52:13:59.1: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:21:25.15 +52:13:59.1: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 21 25.15 +52 13 59.1 12.5 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,2461235.6690,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.51 23:43:42.88 +53:55:36.1
112.96928 -7.62990 galactic Cas Second-epoch detections are separated by 2.4" 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 1993384035355091200 | 23:43:43.12 +53:55:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:43:42.88 +53:55:36.1: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:43:42.88 +53:55:36.1: 13.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 43 42.88 +53 55 36.1 12.5 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 1993384035355091200,2461235.6690,12.51,0.05,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
Gaia DR3 1993384035355091200 20260714.1690 12.51CV 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 07 14.1690 2461235.6690 12.53 23:24:16.99 +54:08:47.4
110.29063 -6.57224 galactic Cas Second-epoch detections are separated by 1.2" 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 | ATO J351.0706+54.1467 | 23:24:16.99 +54:08:47.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.445+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:24:16.99 +54:08:47.4: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:24:16.99 +54:08:47.4: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 24 16.99 +54 08 47.4 12.5 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 J351.0706+54.1467,2461235.6690,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.0706+54.1467 20260714.1690 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.61 23:17:09.99 +56:15:31.3
110.06453 -4.23971 galactic Cas Second-epoch detections are separated by 1.4" 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 | 23:17:09.99 +56:15:31.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:17:09.99 +56:15:31.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:17:09.99 +56:15:31.3: 13.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 17 09.99 +56 15 31.3 12.6 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,2461235.6690,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.57 23:53:10.35 +53:59:59.2
114.34873 -7.89813 galactic Cas Second-epoch detections are separated by 3.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:53:10.35 +53:59:59.2 (user input) | T | P | (position from user input) J-Ks=0.243+/-0.053 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:53:10.35 +53:59:59.2: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:53:10.35 +53:59:59.2: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 53 10.35 +53 59 59.2 12.6 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,2461235.6690,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260714.1690 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.45 00:23:31.51 +57:49:05.2
119.20850 -4.85170 galactic Cas Second-epoch detections are separated by 1.9" and 7.5 pix
The object was found in VSX 3" Gaia DR3 422087399924551040
Type: ROT
# Max. Min./Amp. JD0 Period
13.920 G 13.940 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:23:31.51 +57:49:05.2: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:31.51 +57:49:05.2: 13.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 23 31.51 +57 49 05.2 12.4 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 422087399924551040,2461235.6690,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 422087399924551040 20260714.1690 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.53 23:43:39.23 +56:09:51.3
113.54871 -5.46764 galactic Cas Second-epoch detections are separated by 1.7" 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 | target | 23:43:39.23 +56:09:51.3 (user input) | T | P | (position from user input) J-Ks=0.300+/-0.040 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:43:39.23 +56:09:51.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:43:39.23 +56:09:51.3: 13.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 43 39.23 +56 09 51.3 12.5 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,2461235.6690,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.32 23:58:11.78 +57:33:41.6
115.81548 -4.57269 galactic Cas Second-epoch detections are separated by 2.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1998117226749626496 | 23:58:08.48 +57:33:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.542+/-0.038 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:11.78 +57:33:41.6: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:11.78 +57:33:41.6: 13.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 58 11.78 +57 33 41.6 12.3 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 1998117226749626496,2461235.6690,12.32,0.05,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 1998117226749626496 20260714.1690 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.47 23:37:18.44 +52:28:49.3
111.63684 -8.75809 galactic Cas Second-epoch detections are separated by 1.7" 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 | ATO J354.3195+52.4891 | 23:37:18.44 +52:28:49.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.656+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:37:18.44 +52:28:49.3: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:37:18.44 +52:28:49.3: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 37 18.44 +52 28 49.3 12.5 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 J354.3195+52.4891,2461235.6690,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.3195+52.4891 20260714.1690 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.34 23:55:59.53 +54:35:43.1
114.88608 -7.40798 galactic Cas Second-epoch detections are separated by 1.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993647608903859072 | 23:56:02.16 +54:35:53.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.302+/-0.038 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:55:59.53 +54:35:43.1: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:55:59.53 +54:35:43.1: 13.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 55 59.53 +54 35 43.1 12.3 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 1993647608903859072,2461235.6690,12.34,0.05,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 1993647608903859072 20260714.1690 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.36 23:50:53.38 +53:45:32.0
113.96213 -8.05505 galactic Cas Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993473168814564224 | 23:50:55.45 +53:45:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.433+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:50:53.38 +53:45:32.0: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:50:53.38 +53:45:32.0: 13.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 50 53.38 +53 45 32.0 12.4 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 1993473168814564224,2461235.6690,12.36,0.05,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 1993473168814564224 20260714.1690 12.36CV 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 07 14.1690 2461235.6690 12.41 23:35:48.73 +53:57:55.9
111.85308 -7.27151 galactic Cas Second-epoch detections are separated by 2.3" and 7.2 pix
The object was found in VSX 2" Gaia DR3 1994094873921227648
Type: ROT
# Max. Min./Amp. JD0 Period
14.270 G 14.330 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:35:48.73 +53:57:55.9: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:35:48.73 +53:57:55.9: 13.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 35 48.73 +53 57 55.9 12.4 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 1994094873921227648,2461235.6690,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994094873921227648 20260714.1690 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.27 00:03:11.56 +53:21:29.4
115.68155 -8.83305 galactic Cas Second-epoch detections are separated by 2.2" and 7.5 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 396249701302810752 | 00:03:08.61 +53:20:54.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.188+/-0.038 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:03:11.56 +53:21:29.4: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:03:11.56 +53:21:29.4: 13.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 03 11.56 +53 21 29.4 12.3 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 396249701302810752,2461235.6690,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 396249701302810752 20260714.1690 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.42 23:45:22.60 +56:43:43.9
113.92559 -4.98328 galactic Cas Second-epoch detections are separated by 6.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.3388+56.7292 | 23:45:22.60 +56:43:43.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:45:22.60 +56:43:43.9: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:45:22.60 +56:43:43.9: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 45 22.60 +56 43 43.9 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.3388+56.7292,2461235.6690,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.3388+56.7292 20260714.1690 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.16 00:17:55.26 +57:40:39.0
118.44666 -4.90207 galactic Cas Second-epoch detections are separated by 3.1" 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 | target | 00:17:55.26 +57:40:39.0 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.392+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:55.26 +57:40:39.0: 13.76 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:55.26 +57:40:39.0: 13.48 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.76 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 17 55.26 +57 40 39.0 12.2 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,2461235.6690,12.16,0.05,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 20260714.1690 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.35 23:32:17.21 +53:33:23.2
111.22883 -7.50718 galactic Cas Second-epoch detections are separated by 2.6" 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 | ATO J353.0553+53.5633 | 23:32:17.21 +53:33:23.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.978+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:32:17.21 +53:33:23.2: 13.71 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:32:17.21 +53:33:23.2: 13.38 +/- 0.32 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 32 17.21 +53 33 23.2 12.3 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 J353.0553+53.5633,2461235.6690,12.35,0.05,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
ATO J353.0553+53.5633 20260714.1690 12.35CV 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 07 14.1690 2461235.6690 12.23 23:42:19.55 +53:35:56.3
112.68212 -7.89176 galactic Cas Second-epoch detections are separated by 1.8" and 7.3 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 | 23:42:19.55 +53:35:56.3 (user input) | T | P | (position from user input) J-Ks=0.717+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:42:19.55 +53:35:56.3: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:42:19.55 +53:35:56.3: 13.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 42 19.55 +53 35 56.3 12.2 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,2461235.6690,12.23,0.05,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 20260714.1690 12.23CV 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 07 14.1690 2461235.6690 12.06 23:51:53.10 +53:41:36.0
114.09133 -8.15308 galactic Cas Second-epoch detections are separated by 1.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J357.9751+53.6901 | 23:51:53.10 +53:41:36.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.719+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:53.10 +53:41:36.0: 13.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:53.10 +53:41:36.0: 13.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 51 53.10 +53 41 36.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.9751+53.6901,2461235.6690,12.06,0.05,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
ATO J357.9751+53.6901 20260714.1690 12.06CV 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 07 14.1690 2461235.6690 12.32 23:29:13.57 +52:52:54.0
110.57827 -8.00687 galactic Cas Second-epoch detections are separated by 0.9" and 7.2 pix
The object was found in VSX 1" Gaia DR3 1992477767192633088
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.930 G 13.960 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:13.57 +52:52:54.0: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:13.57 +52:52:54.0: 13.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 29 13.57 +52 52 54.0 12.3 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 1992477767192633088,2461235.6690,12.32,0.05,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 1992477767192633088 20260714.1690 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.23 23:43:42.98 +55:12:23.4
113.30624 -6.39457 galactic Cas Second-epoch detections are separated by 3.4" 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 J355.9453+55.2041 | 23:43:45.58 +55:12:12.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:43:42.98 +55:12:23.4: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:43:42.98 +55:12:23.4: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 43 42.98 +55 12 23.4 12.2 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 J355.9453+55.2041,2461235.6690,12.23,0.05,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
ATO J355.9453+55.2041 20260714.1690 12.23CV 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 07 14.1690 2461235.6690 12.20 23:49:33.33 +55:08:08.6
114.10097 -6.67146 galactic Cas Second-epoch detections are separated by 0.9" 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 | ATO J357.3963+55.1344 | 23:49:33.33 +55:08:08.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.402+/-0.040 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:49:33.33 +55:08:08.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:49:33.33 +55:08:08.6: 13.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 49 33.33 +55 08 08.6 12.2 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 J357.3963+55.1344,2461235.6690,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.3963+55.1344 20260714.1690 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.04 23:52:21.38 +51:55:18.8
113.74779 -9.89319 galactic Cas Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:52:21.38 +51:55:18.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.468+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:52:21.38 +51:55:18.8: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:52:21.38 +51:55:18.8: 13.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 52 21.38 +51 55 18.8 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461235.6690,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.26 23:36:09.08 +55:02:17.9
112.21358 -6.25902 galactic Cas Second-epoch detections are separated by 2.2" and 7.3 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 J354.0422+55.0343 | 23:36:09.08 +55:02:17.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.202+/-0.036 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:36:09.08 +55:02:17.9: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:36:09.08 +55:02:17.9: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 36 09.08 +55 02 17.9 12.3 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 J354.0422+55.0343,2461235.6690,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.0422+55.0343 20260714.1690 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.97 00:04:35.68 +54:16:59.0
116.06031 -7.96252 galactic Cas Second-epoch detections are separated by 1.1" and 7.4 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 | 00:04:35.68 +54:16:59.0 (user input) | T | P | (position from user input) J-Ks=0.259+/-0.034 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:04:35.68 +54:16:59.0: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:04:35.68 +54:16:59.0: 13.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 04 35.68 +54 16 59.0 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461235.6690,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.09 23:30:49.93 +57:02:05.0
112.09915 -4.13202 galactic Cas Second-epoch detections are separated by 3.4" 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 | target | 23:30:49.93 +57:02:05.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:30:49.93 +57:02:05.0: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:30:49.93 +57:02:05.0: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 30 49.93 +57 02 05.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461235.6690,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.95 23:32:07.88 +50:45:59.5
110.34399 -10.15668 galactic Cas Second-epoch detections are separated by 1.2" and 7.5 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 J353.0353+50.7556 | 23:32:07.88 +50:45:59.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.282+/-0.035 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:32:07.88 +50:45:59.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:32:07.88 +50:45:59.5: 13.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 32 07.88 +50 45 59.5 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.0353+50.7556,2461235.6690,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.0353+50.7556 20260714.1690 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.90 23:57:47.02 +56:40:02.3
115.57512 -5.43611 galactic Cas Second-epoch detections are separated by 0.5" 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 | ATO J359.4451+56.6691 | 23:57:43.94 +56:39:42.8 (Gaia DR3) | DBH (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:47.02 +56:40:02.3: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:47.02 +56:40:02.3: 12.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 57 47.02 +56 40 02.3 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.4451+56.6691,2461235.6690,11.90,0.05,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 J359.4451+56.6691 20260714.1690 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.12 23:30:42.49 +51:34:34.0
110.38247 -9.31779 galactic Cas Second-epoch detections are separated by 1.3" and 7.2 pix
The object was found in VSX19" Gaia DR3 1991410691157947520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.020 G 13.050 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:30:42.49 +51:34:34.0: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:30:42.49 +51:34:34.0: 13.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 30 42.49 +51 34 34.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991410691157947520,2461235.6690,12.12,0.05,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 1991410691157947520 20260714.1690 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.74 00:02:42.98 +50:56:43.9
115.14371 -11.18798 galactic Cas Second-epoch detections are separated by 0.8" and 7.5 pix
The object was found in VSX12" Gaia DR3 394042878388217984
Type: ROT
# Max. Min./Amp. JD0 Period
13.220 G 13.270 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:02:42.98 +50:56:43.9: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:02:42.98 +50:56:43.9: 13.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 02 42.98 +50 56 43.9 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 394042878388217984,2461235.6690,11.74,0.05,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
Gaia DR3 394042878388217984 20260714.1690 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 07 14.1690 2461235.6690 12.07 23:42:27.42 +53:50:34.9
112.76665 -7.66171 galactic Cas Second-epoch detections are separated by 1.2" and 6.9 pix
The object was found in VSX22" Gaia DR3 1993378370296817024
Type: ROT
# Max. Min./Amp. JD0 Period
15.490 G 15.530 G F
ATTENTION: measured mag 12.07 is 3.4 mag brighter than the VSX record maximum brightness 15.49 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:42:27.42 +53:50:34.9: 13.62 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:42:27.42 +53:50:34.9: 13.07 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 42 27.42 +53 50 34.9 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993378370296817024,2461235.6690,12.07,0.05,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 1993378370296817024 20260714.1690 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.77 00:07:17.90 +57:21:29.9
116.98330 -5.00275 galactic Cas Second-epoch detections are separated by 2.0" 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 | ATO J001.8287+57.3578 | 00:07:17.90 +57:21:29.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:17.90 +57:21:29.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:17.90 +57:21:29.9: 13.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 07 17.90 +57 21 29.9 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
ATO J001.8287+57.3578,2461235.6690,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.8287+57.3578 20260714.1690 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.70 23:45:04.99 +50:54:58.6
112.38072 -10.59106 galactic Cas Second-epoch detections are separated by 1.0" and 7.4 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 | 23:45:04.99 +50:54:58.6 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:45:04.99 +50:54:58.6: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:45:04.99 +50:54:58.6: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 45 04.99 +50 54 58.6 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,2461235.6690,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.75 23:46:34.48 +57:42:57.7
114.33211 -4.06865 galactic Cas Second-epoch detections are separated by 0.5" 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 J356.6458+57.7147 | 23:46:34.48 +57:42:57.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.413+/-0.056 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:46:34.48 +57:42:57.7: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:34.48 +57:42:57.7: 13.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 46 34.48 +57 42 57.7 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
ATO J356.6458+57.7147,2461235.6690,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J356.6458+57.7147 20260714.1690 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.66 23:19:47.50 +56:13:02.4
110.39226 -4.40686 galactic Cas Second-epoch detections are separated by 1.7" 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 | Gaia DR3 1997181924616091136 | 23:19:49.34 +56:13:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.319+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:19:47.50 +56:13:02.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:19:47.50 +56:13:02.4: 13.05 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 19 47.50 +56 13 02.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997181924616091136,2461235.6690,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997181924616091136 20260714.1690 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.29 00:11:44.35 +50:55:14.3
116.56696 -11.45984 galactic Cas Second-epoch detections are separated by 2.3" and 7.3 pix
The object was found in VSX18" Gaia DR3 395358306610419456
Type: RS
# Max. Min./Amp. JD0 Period
11.860 G 12.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:11:44.35 +50:55:14.3: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:11:44.35 +50:55:14.3: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 11 44.35 +50 55 14.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395358306610419456,2461235.6690,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 395358306610419456 20260714.1690 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.57 23:51:16.14 +53:25:17.0
113.93759 -8.39635 galactic Cas Second-epoch detections are separated by 2.2" and 6.9 pix
The object was found in VSX 1" Gaia DR3 1945411522700076672
Type: ROT
# Max. Min./Amp. JD0 Period
13.500 G 13.540 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:16.14 +53:25:17.0: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:16.14 +53:25:17.0: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 51 16.14 +53 25 17.0 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
Gaia DR3 1945411522700076672,2461235.6690,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1945411522700076672 20260714.1690 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.35 00:27:07.04 +53:23:25.1
119.26196 -9.30805 galactic Cas Second-epoch detections are separated by 0.6" and 7.4 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 419427234618930944 | 00:27:02.46 +53:23:21.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.181+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:07.04 +53:23:25.1: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:07.04 +53:23:25.1: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 27 07.04 +53 23 25.1 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 419427234618930944,2461235.6690,11.35,0.05,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 419427234618930944 20260714.1690 11.35CV 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 07 14.1690 2461235.6690 11.45 23:22:56.28 +55:56:21.0
110.71067 -4.81836 galactic Cas Second-epoch detections are separated by 1.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1997022117471714688 | 23:22:55.58 +55:56:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.476+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:22:56.28 +55:56:21.0: 13.29 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:22:56.28 +55:56:21.0: 13.37 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 22 56.28 +55 56 21.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997022117471714688,2461235.6690,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1997022117471714688 20260714.1690 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.42 23:10:02.60 +56:51:39.6
109.37348 -3.31764 galactic Cas Second-epoch detections are separated by 4.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J347.5055+56.8648 | 23:10:04.48 +56:52:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:10:02.60 +56:51:39.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:10:02.60 +56:51:39.6: 13.31 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 10 02.60 +56 51 39.6 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.5055+56.8648,2461235.6690,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.5055+56.8648 20260714.1690 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.13 23:45:23.29 +53:48:02.7
113.17696 -7.81532 galactic Cas Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993704959608606336 | 23:45:25.30 +53:48:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.394+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:45:23.29 +53:48:02.7: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:45:23.29 +53:48:02.7: 13.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 45 23.29 +53 48 02.7 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 1993704959608606336,2461235.6690,11.13,0.05,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
Gaia DR3 1993704959608606336 20260714.1690 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 07 14.1690 2461235.6690 10.98 00:17:52.69 +57:46:42.6
118.45417 -4.80118 galactic Cas Second-epoch detections are separated by 0.7" 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 422057640085161600 | 00:17:51.02 +57:46:55.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.128+/-0.027 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:52.69 +57:46:42.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:52.69 +57:46:42.6: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 17 52.69 +57 46 42.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 422057640085161600,2461235.6690,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 422057640085161600 20260714.1690 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 9.97 23:51:09.65 +55:30:06.1
114.41124 -6.36970 galactic Cas Second-epoch detections are separated by 1.0" 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 1994651432965279360 | 23:51:10.21 +55:30:22.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.236+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:09.65 +55:30:06.1: 11.37 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:09.65 +55:30:06.1: 11.06 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.21 +/- 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 07 14.1690* 23 51 09.65 +55 30 06.1 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994651432965279360,2461235.6690,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994651432965279360 20260714.1690 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 10.30 23:59:07.22 +54:42:32.6
115.35621 -7.39133 galactic Cas Second-epoch detections are separated by 0.7" and 7.3 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 1993662972011235072 | 23:59:02.79 +54:42:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.232+/-0.032 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:07.22 +54:42:32.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:07.22 +54:42:32.6: 13.41 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 59 07.22 +54 42 32.6 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 1993662972011235072,2461235.6690,10.30,0.05,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
Gaia DR3 1993662972011235072 20260714.1690 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.46 23:25:04.93 +55:05:34.5
110.71530 -5.71737 galactic Cas Second-epoch detections are separated by 1.7" 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 | 23:25:04.93 +55:05:34.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.363+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:04.93 +55:05:34.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:04.93 +55:05:34.5: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 25 04.93 +55 05 34.5 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
target,2461235.6690,11.46,0.05,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
target 20260714.1690 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.54 23:56:52.64 +52:09:35.2
114.48938 -9.81534 galactic Cas Second-epoch detections are separated by 0.7" and 7.3 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 | 23:56:52.64 +52:09:35.2 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:56:52.64 +52:09:35.2: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:56:52.64 +52:09:35.2: 13.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 56 52.64 +52 09 35.2 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461235.6690,11.54,0.05,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
target 20260714.1690 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 07 14.1690 2461235.6690 11.87 23:19:31.89 +55:36:23.6
110.14463 -4.96675 galactic Cas Second-epoch detections are separated by 4.3" and 7.4 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 1996916972372159360 | 23:19:35.92 +55:36:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.852+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:19:31.89 +55:36:23.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:19:31.89 +55:36:23.6: 13.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 19 31.89 +55 36 23.6 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996916972372159360,2461235.6690,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996916972372159360 20260714.1690 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.62 23:33:40.95 +49:58:06.8
110.33676 -10.99208 galactic And Second-epoch detections are separated by 1.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.4219+49.9732 | 23:33:43.36 +49:58:40.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 1952CoRut..32....1H BD+49 4154 J-Ks=0.388+/-0.031 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:33:40.95 +49:58:06.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:33:40.95 +49:58:06.8: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 33 40.95 +49 58 06.8 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J353.4219+49.9732,2461235.6690,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.4219+49.9732 20260714.1690 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.79 23:35:43.42 +53:18:09.8
111.64578 -7.90179 galactic Cas Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993255637311656448 | 23:35:39.17 +53:18:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.570+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:35:43.42 +53:18:09.8: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:35:43.42 +53:18:09.8: 13.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 35 43.42 +53 18 09.8 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
Gaia DR3 1993255637311656448,2461235.6690,11.79,0.05,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
Gaia DR3 1993255637311656448 20260714.1690 11.79CV 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 07 14.1690 2461235.6690 11.72 00:09:09.21 +49:47:10.2
115.96314 -12.51257 galactic Cas Second-epoch detections are separated by 2.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 393729105252457472 | 00:09:09.64 +49:46:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2 1958PMcCO..13b....V AG+49 24
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:09:09.21 +49:47:10.2: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:09:09.21 +49:47:10.2: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 09 09.21 +49 47 10.2 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393729105252457472,2461235.6690,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 393729105252457472 20260714.1690 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.10 23:14:42.28 +56:55:19.2
109.98781 -3.49880 galactic Cas Second-epoch detections are separated by 1.2" 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 | ASASSN-V J231436.71+565516.1 | 23:14:36.72 +56:55:16.2 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.410+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:14:42.28 +56:55:19.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:14:42.28 +56:55:19.2: 13.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 14 42.28 +56 55 19.2 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J231436.71+565516.1,2461235.6690,12.10,0.05,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
ASASSN-V J231436.71+565516.1 20260714.1690 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.97 23:28:09.68 +52:54:27.8
110.43285 -7.93118 galactic Cas Second-epoch detections are separated by 1.4" and 7.3 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 1992527039058909440 | 23:28:08.76 +52:53:44.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:09.68 +52:54:27.8: 13.63 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:09.68 +52:54:27.8: 13.52 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.63 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 28 09.68 +52 54 27.8 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992527039058909440,2461235.6690,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992527039058909440 20260714.1690 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.91 23:14:47.95 +52:51:33.5
108.50623 -7.28440 galactic And Second-epoch detections are separated by 4.6" and 6.3 pix
The object was found in VSX 5" Gaia DR3 1995292207724496512
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.800 G 13.850 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:14:47.95 +52:51:33.5: 13.48 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:14:47.95 +52:51:33.5: 13.32 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.48 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 14 47.95 +52 51 33.5 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1995292207724496512,2461235.6690,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995292207724496512 20260714.1690 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.07 23:25:48.89 +51:50:37.5
109.74191 -8.82170 galactic And Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1991651690363076352 | 23:25:44.83 +51:50:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:48.89 +51:50:37.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:48.89 +51:50:37.5: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 25 48.89 +51 50 37.5 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1991651690363076352,2461235.6690,12.07,0.05,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 1991651690363076352 20260714.1690 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 11.97 23:29:20.99 +51:14:37.8
110.07289 -9.56682 galactic Cas Second-epoch detections are separated by 4.3" 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 | 23:29:20.99 +51:14:37.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:20.99 +51:14:37.8: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:20.99 +51:14:37.8: 13.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 29 20.99 +51 14 37.8 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461235.6690,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.04 23:57:00.77 +53:44:34.5
114.84987 -8.27261 galactic Cas Second-epoch detections are separated by 0.3" 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 | target | 23:57:00.77 +53:44:34.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:00.77 +53:44:34.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:00.77 +53:44:34.5: 13.33 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 57 00.77 +53 44 34.5 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461235.6690,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.38 23:33:49.55 +55:18:17.4
111.97288 -5.90690 galactic Cas Second-epoch detections are separated by 2.0" and 6.6 pix
The object was found in VSX 7" V0437 Cas
Type: M
# Max. Min./Amp. JD0 Period
14.400 B < 17.100 B 2441170.00000 266.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:33:49.55 +55:18:17.4: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:33:49.55 +55:18:17.4: 13.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 33 49.55 +55 18 17.4 12.4 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
V0437 Cas,2461235.6690,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0437 Cas 20260714.1690 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.51 23:11:59.48 +56:58:23.3
109.66246 -3.31438 galactic Cas Second-epoch detections are separated by 1.6" 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 | 23:11:59.48 +56:58:23.3 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:11:59.48 +56:58:23.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:11:59.48 +56:58:23.3: 13.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 11 59.48 +56 58 23.3 12.5 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,2461235.6690,12.51,0.05,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 20260714.1690 12.51CV 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 07 14.1690 2461235.6690 12.38 00:28:05.53 +57:36:00.0
119.79588 -5.12953 galactic Cas Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.0355+57.5891 | 00:28:05.53 +57:36:00.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.576+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:05.53 +57:36:00.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:05.53 +57:36:00.0: 13.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 28 05.53 +57 36 00.0 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J007.0355+57.5891,2461235.6690,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J007.0355+57.5891 20260714.1690 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.40 23:10:53.96 +56:47:38.6
109.45647 -3.42408 galactic Cas Second-epoch detections are separated by 2.4" 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 J347.7388+56.7999 | 23:10:57.32 +56:47:59.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M4 (LAMOST DR5) J-Ks=0.426+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:10:53.96 +56:47:38.6: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:10:53.96 +56:47:38.6: 13.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 10 53.96 +56 47 38.6 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.7388+56.7999,2461235.6690,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.7388+56.7999 20260714.1690 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.23 23:24:08.33 +56:51:15.0
111.17428 -4.01141 galactic Cas Second-epoch detections are separated by 0.1" 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 J351.0321+56.8609 | 23:24:10.70 +56:51:52.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:24:08.33 +56:51:15.0: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:24:08.33 +56:51:15.0: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 24 08.33 +56 51 15.0 12.2 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 J351.0321+56.8609,2461235.6690,12.23,0.05,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
ATO J351.0321+56.8609 20260714.1690 12.23CV 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 07 14.1690 2461235.6690 12.40 23:25:59.04 +51:16:49.6
109.57957 -9.36235 galactic Cas Second-epoch detections are separated by 1.3" and 7.4 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 | 23:25:59.04 +51:16:49.6 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.063 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:59.04 +51:16:49.6: 13.51 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:59.04 +51:16:49.6: 13.49 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.51 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 25 59.04 +51 16 49.6 12.4 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,2461235.6690,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.29 00:07:17.52 +58:04:10.9
117.10446 -4.30169 galactic Cas Second-epoch detections are separated by 2.1" and 7.3 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 J001.8071+58.0668 | 00:07:13.54 +58:04:30.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1948PMcCO..10...57V BD+57 2869 J-Ks=0.350+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:17.52 +58:04:10.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:17.52 +58:04:10.9: 13.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 07 17.52 +58 04 10.9 12.3 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 J001.8071+58.0668,2461235.6690,12.29,0.05,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
ATO J001.8071+58.0668 20260714.1690 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.65 23:21:02.63 +55:32:43.1
110.32466 -5.09818 galactic Cas Second-epoch detections are separated by 2.4" 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 | 23:21:02.63 +55:32:43.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:21:02.63 +55:32:43.1: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:21:02.63 +55:32:43.1: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 21 02.63 +55 32 43.1 12.7 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,2461235.6690,12.65,0.05,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 20260714.1690 12.65CV 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 07 14.1690 2461235.6690 12.45 23:31:47.05 +52:31:41.9
110.83934 -8.46322 galactic Cas Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993196194963660672 | 23:31:43.28 +52:31:53.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.365+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:31:47.05 +52:31:41.9: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:31:47.05 +52:31:41.9: 13.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 31 47.05 +52 31 41.9 12.4 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 1993196194963660672,2461235.6690,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1993196194963660672 20260714.1690 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.73 23:25:04.90 +57:12:06.6
111.41062 -3.72554 galactic Cas Second-epoch detections are separated by 0.3" 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 | 23:25:04.90 +57:12:06.6 (user input) | T | P | (position from user input) J-Ks=1.028+/-0.033 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:04.90 +57:12:06.6: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:04.90 +57:12:06.6: 13.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 25 04.90 +57 12 06.6 12.7 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,2461235.6690,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.62 23:20:53.67 +56:39:59.8
110.69129 -4.03789 galactic Cas Second-epoch detections are separated by 1.5" 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 | target | 23:20:53.67 +56:39:59.8 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.031 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:20:53.67 +56:39:59.8: 13.59 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:20:53.67 +56:39:59.8: 13.43 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.59 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 20 53.67 +56 39 59.8 12.6 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,2461235.6690,12.62,0.05,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
target 20260714.1690 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.77 23:13:34.42 +55:35:38.4
109.35204 -4.67612 galactic Cas Second-epoch detections are separated by 0.8" and 6.9 pix
The object was found in VSX 2" Gaia DR3 1997136810278664832
Type: ROT
# Max. Min./Amp. JD0 Period
14.040 G 14.070 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:13:34.42 +55:35:38.4: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:13:34.42 +55:35:38.4: 13.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 13 34.42 +55 35 38.4 12.8 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 1997136810278664832,2461235.6690,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997136810278664832 20260714.1690 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.69 23:17:02.07 +54:44:50.6
109.50480 -5.64450 galactic Cas Second-epoch detections are separated by 1.3" and 6.6 pix
The object was found in VSX16" Gaia DR3 1996798362556720896
Type: ROT
# Max. Min./Amp. JD0 Period
16.370 G 16.410 G K
ATTENTION: measured mag 12.69 is 3.7 mag brighter than the VSX record maximum brightness 16.37 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:17:02.07 +54:44:50.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:17:02.07 +54:44:50.6: 13.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 17 02.07 +54 44 50.6 12.7 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 1996798362556720896,2461235.6690,12.69,0.05,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 1996798362556720896 20260714.1690 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.72 23:32:53.70 +54:41:15.1
111.65903 -6.45601 galactic Cas Second-epoch detections are separated by 0.8" 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 | ATO J353.2360+54.6815 | 23:32:53.70 +54:41:15.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.695+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:32:53.70 +54:41:15.1: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:32:53.70 +54:41:15.1: 13.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 32 53.70 +54 41 15.1 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.2360+54.6815,2461235.6690,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J353.2360+54.6815 20260714.1690 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.72 00:17:21.92 +58:13:32.3
118.44549 -4.34900 galactic Cas Second-epoch detections are separated by 1.4" 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 | 00:17:21.92 +58:13:32.3 (user input) | T | P | (position from user input) J-Ks=0.563+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:21.92 +58:13:32.3: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:21.92 +58:13:32.3: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 17 21.92 +58 13 32.3 12.7 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,2461235.6690,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260714.1690 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.64 23:55:53.24 +57:04:30.3
115.40716 -4.98286 galactic Cas Second-epoch detections are separated by 1.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J358.9522+57.0810 | 23:55:53.24 +57:04:30.3 (user input) | PULSE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.840+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:55:53.24 +57:04:30.3: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:55:53.24 +57:04:30.3: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 55 53.24 +57 04 30.3 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.9522+57.0810,2461235.6690,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.9522+57.0810 20260714.1690 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.60 23:37:17.75 +53:04:18.5
111.80619 -8.19086 galactic Cas Second-epoch detections are separated by 2.9" and 7.6 pix
The object was found in VSX 3" Gaia DR3 1993192381031958272
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.440 G 14.470 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:37:17.75 +53:04:18.5: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:37:17.75 +53:04:18.5: 13.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 37 17.75 +53 04 18.5 12.6 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 1993192381031958272,2461235.6690,12.60,0.05,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 1993192381031958272 20260714.1690 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.79 00:14:09.17 +57:57:33.4
117.98683 -4.55404 galactic Cas Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:14:09.17 +57:57:33.4 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:14:09.17 +57:57:33.4: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:14:09.17 +57:57:33.4: 13.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 14 09.17 +57 57 33.4 12.8 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,2461235.6690,12.79,0.05,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 20260714.1690 12.79CV 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 07 14.1690 2461235.6690 12.76 23:49:01.53 +56:53:05.0
114.44998 -4.95567 galactic Cas Second-epoch detections are separated by 1.5" 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 | 23:49:01.53 +56:53:05.0 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.046 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:49:01.53 +56:53:05.0: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:49:01.53 +56:53:05.0: 13.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 49 01.53 +56 53 05.0 12.8 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,2461235.6690,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.72 23:29:19.10 +53:25:13.0
110.76283 -7.50007 galactic Cas Second-epoch detections are separated by 1.6" 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 | target | 23:29:19.10 +53:25:13.0 (user input) | T | P | (position from user input) J-Ks=0.256+/-0.039 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:19.10 +53:25:13.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:19.10 +53:25:13.0: 13.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 29 19.10 +53 25 13.0 12.7 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,2461235.6690,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260714.1690 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.84 23:44:55.96 +55:59:33.2
113.67735 -5.67958 galactic Cas Second-epoch detections are separated by 1.6" 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 | ATO J356.2458+56.0037 | 23:44:58.32 +56:00:01.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.575+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:44:55.96 +55:59:33.2: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:44:55.96 +55:59:33.2: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 44 55.96 +55 59 33.2 12.8 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 J356.2458+56.0037,2461235.6690,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.2458+56.0037 20260714.1690 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.74 00:02:10.03 +57:51:20.3
116.39530 -4.38944 galactic Cas Second-epoch detections are separated by 1.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:02:10.03 +57:51:20.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:02:10.03 +57:51:20.3: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:02:10.03 +57:51:20.3: 13.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 02 10.03 +57 51 20.3 12.7 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,2461235.6690,12.74,0.05,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 20260714.1690 12.74CV 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 07 14.1690 2461235.6690 12.73 23:46:41.19 +54:17:34.0
113.48844 -7.38744 galactic Cas Second-epoch detections are separated by 0.6" 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 | target | 23:46:41.19 +54:17:34.0 (user input) | T | P | (position from user input) J-Ks=0.827+/-0.035 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:46:41.19 +54:17:34.0: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:41.19 +54:17:34.0: 13.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 46 41.19 +54 17 34.0 12.7 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,2461235.6690,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.68 00:21:08.08 +55:12:51.0
118.58203 -7.40144 galactic Cas Second-epoch detections are separated by 1.4" 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 | 00:21:08.08 +55:12:51.0 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:21:08.08 +55:12:51.0: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:21:08.08 +55:12:51.0: 13.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 21 08.08 +55 12 51.0 12.7 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,2461235.6690,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 14.1690 2461235.6690 12.88 00:05:58.74 +53:50:18.5
116.18141 -8.43639 galactic Cas Second-epoch detections are separated by 2.1" and 7.5 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 | 00:05:58.74 +53:50:18.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:05:58.74 +53:50:18.5: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:05:58.74 +53:50:18.5: 13.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 00 05 58.74 +53 50 18.5 12.9 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,2461235.6690,12.88,0.05,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 20260714.1690 12.88CV 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 07 14.1690 2461235.6690 11.80 23:28:54.71 +54:18:51.1
110.98949 -6.63284 galactic Cas Second-epoch detections are separated by 1.1" 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 | target | 23:28:54.71 +54:18:51.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:54.71 +54:18:51.1: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:54.71 +54:18:51.1: 13.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 14.1690* 23 28 54.71 +54 18 51.1 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,2461235.6690,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260714.1690 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
First image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461235.66924172 14.07.2026 04:03:32.485 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.79
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 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): 17351
Objects passed selection criteria: 17329
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 15750.5
Average stars matched: 15398.5 (97.7652 %)
Memory usage VmPeak: 126596 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jul 13 18:59:08 CDT 2026
VaST build number 1.0rc89-151-g9f3411f7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jul 14 00:21:49 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
First image: 2461206.83945590 15.06.2026 08:08:38.990 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461235.66924172 14.07.2026 04:03:32.485 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 211
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 215 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): 137806
Objects passed selection criteria: 137505
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 128341
Average stars matched: 124518 (97.0214 %)
Memory usage VmPeak: 1971124 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jul 13 18:59:08 CDT 2026
VaST build number 1.0rc89-151-g9f3411f7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jul 14 00:29:37 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 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.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: 2461235.66869972
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Image size: 927.0'x616.4' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:01.466 +54:00:23.28 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
Image size: 939.7'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:04.757 +53:59:44.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 00:00:04.757 +53:59:44.56
Angular distance between the image centers 0.0134 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
Image size: 939.6'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:08.281 +54:00:14.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 00:00:08.281 +54:00:14.38
Angular distance between the image centers 0.0169 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 00:00:04.757 +53:59:44.56
Second-epoch second image center 00:00:08.281 +54:00:14.38
Angular distance between the image centers 0.01196 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits &> /tmp/tmp.PCjz4Zxecf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits &> /tmp/tmp.VT1OyiSGGx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits &> /tmp/tmp.4u3DJxZyOM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits &> /tmp/tmp.OPHlKYSh2Q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 23386 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0031 to 359.9999 deg, Dec +48.2162 to +59.2586 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0031 to 359.9999 deg, Dec 48.2162 to 59.2586 deg
Loaded 153985 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 53 out of 58 total matches.
Matched with Tycho-2 58 out of 23386 detected stars.
ERROR: only 53 of 23386 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.23%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.473500
a=0.000000 b=1.000000 c=22.473500
From vast_summary.log: estimated ref. image limiting mag.: -7.79
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.68
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23386 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0031 to 359.9999 deg, Dec +48.2162 to +59.2586 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0031 to 359.9999 deg, Dec 48.2162 to 59.2586 deg
Loaded 153985 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 53 out of 58 total matches.
Matched with Tycho-2 58 out of 23386 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (aperture=6.2)
Read 23366 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0031 to 360.0000 deg, Dec +48.2161 to +59.2689 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0031 to 360.0000 deg, Dec 48.2161 to 59.2689 deg
Loaded 154106 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 50 out of 55 total matches.
Matched with Tycho-2 55 out of 23366 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
2.3 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Limiting magnitude estimates:
14.7 mag. Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
14.7 mag. Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
14.3 mag. fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
14.3 mag. fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.PCjz4Zxecf (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1910, bad_region=5051, passed=23386
Got 23386 stars (including 16726 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 23386 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.0'
Seting catalog search parameters based on the expected field of view 927.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012875 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010300 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9996 through 0 to 14.8812, gap 14.8812 to 344.9996
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 325 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 241 matched stars entering correct_measured_positions(), 168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 4908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.09"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9814 through 0 to 14.9033, gap 14.9033 to 344.9814
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 397 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 328 matched stars entering correct_measured_positions(), 4961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.99"
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 6645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.24"
Excluding outliers - 325 stars left (next iteration limit 256)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits N_match=325 sigma_overall_arcsec=11.131 sigma_q1_arcsec=25.602 sigma_q2_arcsec=32.104 sigma_q3_arcsec=8.250 sigma_q4_arcsec=9.745 n_q1=41 n_q2=23 n_q3=116 n_q4=145 worst_quadrant_to_overall_ratio=2.884
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VT1OyiSGGx (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1872, bad_region=4985, passed=23366
Got 23366 stars (including 16797 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 23366 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.1'
Seting catalog search parameters based on the expected field of view 927.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012876 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010301 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0112 through 0 to 14.8810, gap 14.8810 to 345.0112
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 239 matched stars entering correct_measured_positions(), 165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 231 matched stars entering correct_measured_positions(), 4693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9936 through 0 to 14.9023, gap 14.9023 to 344.9936
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 397 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 321 matched stars entering correct_measured_positions(), 4741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.79"
Accuracy estimation diagnostic: 315 matched stars entering correct_measured_positions(), 6313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.43"
Excluding outliers - 315 stars left (next iteration limit 254)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits N_match=315 sigma_overall_arcsec=10.449 sigma_q1_arcsec=28.329 sigma_q2_arcsec=30.359 sigma_q3_arcsec=8.438 sigma_q4_arcsec=7.803 n_q1=34 n_q2=19 n_q3=120 n_q4=142 worst_quadrant_to_overall_ratio=2.905
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4u3DJxZyOM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1172, bad_region=2917, passed=16233
Got 16233 stars (including 12308 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 16233 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (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 0.010441 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8476 through 0 to 14.6559, gap 14.6559 to 344.8476
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13644 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
RA wraps around 0/360 boundary: field RA 344.8478 through 0 to 14.6565, gap 14.6565 to 344.8478
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits N_match=973 sigma_overall_arcsec=0.649 sigma_q1_arcsec=0.750 sigma_q2_arcsec=0.668 sigma_q3_arcsec=0.621 sigma_q4_arcsec=0.661 n_q1=326 n_q2=173 n_q3=287 n_q4=187 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OPHlKYSh2Q (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1157, bad_region=2912, passed=16240
Got 16240 stars (including 12307 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat
util/solve_plate_with_UCAC5 got 16240 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.6'
Seting catalog search parameters based on the expected field of view 939.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013050 (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 0.010440 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8478 through 0 to 14.6563, gap 14.6563 to 344.8478
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8479 through 0 to 14.6567, gap 14.6567 to 344.8479
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits N_match=973 sigma_overall_arcsec=0.633 sigma_q1_arcsec=0.639 sigma_q2_arcsec=0.677 sigma_q3_arcsec=0.655 sigma_q4_arcsec=0.684 n_q1=322 n_q2=173 n_q3=288 n_q4=190 worst_quadrant_to_overall_ratio=1.080
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits sigma_overall=11.131 worst_q_ratio=2.884
ref2=Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits sigma_overall=10.449 worst_q_ratio=2.905
new1=fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits sigma_overall=0.649 worst_q_ratio=1.155
new2=fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits sigma_overall=0.633 worst_q_ratio=1.080
reference average sigma_overall=10.79 worst_q_ratio=2.8945
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006_astrometric_residuals.png (325 matched stars from wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.67 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007_astrometric_residuals.png (315 matched stars from wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.55 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070_astrometric_residuals.png (973 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.59 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071_astrometric_residuals.png (973 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.60 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:36:42.82 +52:12:23.4: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:36:42.82 +52:12:23.4: 15.29 +/- 99.00 upperlimit
Adding exclusion_list_gaiadr2.txt__out31332.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31302_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 31302_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:11:31.19 +56:01:28.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31332_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 31332_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:36:42.82 +52:12:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 1.737 1992951175669473280 354.17773907453 +52.20674593830 10.7215 9.4538 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17508_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 17508_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:44:31.90 +56:34:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05724_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 05724_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:09:36.50 +51:34:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14592_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 14592_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:04:40.70 +55:32:14.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Image size: 927.0'x616.4' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:01.466 +54:00:23.28 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
Image size: 939.7'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:04.757 +53:59:44.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 00:00:04.757 +53:59:44.56
Angular distance between the image centers 0.0134 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
Image size: 939.6'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:08.281 +54:00:14.38 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 00:00:08.281 +54:00:14.38
Angular distance between the image centers 0.0169 deg.
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# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:04.757 +53:59:44.56
Second-epoch second image center 00:00:08.281 +54:00:14.38
Angular distance between the image centers 0.01196 deg.
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Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits &> /tmp/tmp.4JWzCGX4C3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits &> /tmp/tmp.S9Ae3szTfb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits &> /tmp/tmp.1GTghslHXc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits &> /tmp/tmp.LqY2jsBmDk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 167282 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +48.1859 to +59.2631 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0000 to 360.0000 deg, Dec 48.1859 to 59.2631 deg
Loaded 154477 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 105 out of 150 total matches.
Matched with Tycho-2 150 out of 167282 detected stars.
ERROR: only 105 of 167282 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.06%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.702700
a=0.000000 b=1.000000 c=20.702700
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 167282 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +48.1859 to +59.2631 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0000 to 360.0000 deg, Dec 48.1859 to 59.2631 deg
Loaded 154477 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 105 out of 150 total matches.
Matched with Tycho-2 150 out of 167282 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (aperture=4.7)
Read 165704 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +48.1861 to +59.2705 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 0.0000 to 360.0000 deg, Dec 48.1861 to 59.2705 deg
Loaded 154563 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 102 out of 145 total matches.
Matched with Tycho-2 145 out of 165704 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 163 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.2 pix Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
2.1 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Limiting magnitude estimates:
13.3 mag. Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
13.2 mag. Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
12.9 mag. fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
12.9 mag. fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.4JWzCGX4C3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=20826, bad_region=21165, passed=167247
Got 167247 stars (including 127895 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 167247 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.0'
Seting catalog search parameters based on the expected field of view 927.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012875 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010300 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9631 through 0 to 14.9764, gap 14.9764 to 344.9631
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 318 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 216 matched stars entering correct_measured_positions(), 35553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9503 through 0 to 14.9983, gap 14.9983 to 344.9503
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 395 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 320 matched stars entering correct_measured_positions(), 35597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.35"
Accuracy estimation diagnostic: 315 matched stars entering correct_measured_positions(), 52070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.79"
Excluding outliers - 315 stars left (next iteration limit 237)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits N_match=315 sigma_overall_arcsec=8.955 sigma_q1_arcsec=30.923 sigma_q2_arcsec=19.444 sigma_q3_arcsec=6.520 sigma_q4_arcsec=8.008 n_q1=39 n_q2=21 n_q3=117 n_q4=138 worst_quadrant_to_overall_ratio=3.453
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.S9Ae3szTfb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=39, blended=20515, bad_region=20705, passed=165665
Got 165665 stars (including 126839 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 165665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.1'
Seting catalog search parameters based on the expected field of view 927.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012876 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010301 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9474 through 0 to 14.9341, gap 14.9341 to 344.9474
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 326 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 225 matched stars entering correct_measured_positions(), 37244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9404 through 0 to 14.9637, gap 14.9637 to 344.9404
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 400 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 37289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.64"
Accuracy estimation diagnostic: 317 matched stars entering correct_measured_positions(), 52373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.41"
Excluding outliers - 317 stars left (next iteration limit 247)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits N_match=317 sigma_overall_arcsec=8.596 sigma_q1_arcsec=27.471 sigma_q2_arcsec=23.969 sigma_q3_arcsec=6.420 sigma_q4_arcsec=8.419 n_q1=37 n_q2=20 n_q3=128 n_q4=132 worst_quadrant_to_overall_ratio=3.196
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1GTghslHXc (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=12064, bad_region=15586, passed=127521
Got 127521 stars (including 100942 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 127521 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (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 0.010441 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8076 through 0 to 14.7936, gap 14.7936 to 344.8076
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 114071 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
RA wraps around 0/360 boundary: field RA 344.8073 through 0 to 14.7941, gap 14.7941 to 344.8073
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 114073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 114072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits N_match=977 sigma_overall_arcsec=0.642 sigma_q1_arcsec=0.746 sigma_q2_arcsec=0.614 sigma_q3_arcsec=0.644 sigma_q4_arcsec=0.669 n_q1=327 n_q2=175 n_q3=274 n_q4=201 worst_quadrant_to_overall_ratio=1.161
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LqY2jsBmDk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=12297, bad_region=15735, passed=128816
Got 128816 stars (including 101839 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat
util/solve_plate_with_UCAC5 got 128816 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.6'
Seting catalog search parameters based on the expected field of view 939.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013050 (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 0.010440 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.7830 through 0 to 14.7929, gap 14.7929 to 344.7830
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 115276 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.7830 through 0 to 14.7934, gap 14.7934 to 344.7830
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 115276 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 115276 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits N_match=975 sigma_overall_arcsec=0.640 sigma_q1_arcsec=0.676 sigma_q2_arcsec=0.654 sigma_q3_arcsec=0.625 sigma_q4_arcsec=0.661 n_q1=325 n_q2=173 n_q3=279 n_q4=198 worst_quadrant_to_overall_ratio=1.057
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-02-45_20.00sec_5.00C_LIGHT_0070.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_230544_TTUQ2b1x1_1735348_otxfkRrB/wcs_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:23:34.40 +57:25:02.8: 13.16 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:46:24.94 +57:37:52.5: 12.78 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:43:42.88 +53:55:36.1: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:21:25.15 +52:13:59.1: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:03.04 +56:41:42.7: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:09.70 +53:46:57.8: 13.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:24:16.99 +54:08:47.4: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:56:12.73 +54:27:13.9: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:23:34.40 +57:25:02.8: 12.93 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:43:42.88 +53:55:36.1: 13.60 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.06 +/- 0.18
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:24.94 +57:37:52.5: 12.40 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:21:25.15 +52:13:59.1: 13.59 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:23:34.40 +57:25:02.8: ref_mag=13.06 +/- 0.18 new_mean_mag=12.5001 delta=0.56 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:03.04 +56:41:42.7: 13.21 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.57 +/- 0.09
Forced photometry filter REJECTED candidate at 23:46:24.94 +57:37:52.5: ref_mag=12.57 +/- 0.09 new_mean_mag=12.6683 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:24:16.99 +54:08:47.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:09.70 +53:46:57.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:56:12.73 +54:27:13.9: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:11.56 +52:43:47.9: 12.15 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:24:57.71 +54:48:26.6: 13.25 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:54:11.56 +52:43:47.9: 11.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.05
Forced photometry filter REJECTED candidate at 23:54:11.56 +52:43:47.9: ref_mag=11.94 +/- 0.05 new_mean_mag=12.3868 delta=-0.45 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:24:57.71 +54:48:26.6: 13.39 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.25 +/- 0.25
Forced photometry filter REJECTED candidate at 23:24:57.71 +54:48:26.6: ref_mag=13.25 +/- 0.25 new_mean_mag=12.6218 delta=0.63 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:17:09.99 +56:15:31.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:53:10.35 +53:59:59.2: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:17:09.99 +56:15:31.3: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:53:10.35 +53:59:59.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:23:31.51 +57:49:05.2: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:43:39.23 +56:09:51.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:31.51 +57:49:05.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:43:39.23 +56:09:51.3: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:11.78 +57:33:41.6: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:11.78 +57:33:41.6: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:37:18.44 +52:28:49.3: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:37:18.44 +52:28:49.3: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:55:59.53 +54:35:43.1: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:55:59.53 +54:35:43.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:11:08.16 +53:40:31.0: 12.55 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:11:08.16 +53:40:31.0: 12.04 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.07
Forced photometry filter REJECTED candidate at 00:11:08.16 +53:40:31.0: ref_mag=12.24 +/- 0.07 new_mean_mag=12.2115 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:50:53.38 +53:45:32.0: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:41:02.23 +56:51:04.9: 10.57 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:35:48.73 +53:57:55.9: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:03:11.56 +53:21:29.4: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:50:53.38 +53:45:32.0: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:41:02.23 +56:51:04.9: 10.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.37 +/- 0.01
Forced photometry filter REJECTED candidate at 23:41:02.23 +56:51:04.9: ref_mag=10.37 +/- 0.01 new_mean_mag=12.4133 delta=-2.04 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:35:48.73 +53:57:55.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:03:11.56 +53:21:29.4: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:45:22.60 +56:43:43.9: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:55.26 +57:40:39.0: 13.76 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:32:17.21 +53:33:23.2: 13.71 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:45:22.60 +56:43:43.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:42:19.55 +53:35:56.3: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:55.26 +57:40:39.0: 13.48 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.76 +/- 0.36
Forced photometry filter KEPT candidate at 00:17:55.26 +57:40:39.0: ref_mag=13.76 +/- 0.36 new_mean_mag=12.1597 delta=1.60 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:32:17.21 +53:33:23.2: 13.38 +/- 0.32 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.23
Forced photometry filter KEPT candidate at 23:32:17.21 +53:33:23.2: ref_mag=13.55 +/- 0.23 new_mean_mag=12.3463 delta=1.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:42:19.55 +53:35:56.3: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:53.10 +53:41:36.0: 13.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:53.10 +53:41:36.0: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:40:06.43 +54:53:06.0: 12.35 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:13.57 +52:52:54.0: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:40:06.43 +54:53:06.0: 12.16 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.07
Forced photometry filter REJECTED candidate at 23:40:06.43 +54:53:06.0: ref_mag=12.27 +/- 0.07 new_mean_mag=12.1655 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:13.57 +52:52:54.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:43:42.98 +55:12:23.4: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:43:42.98 +55:12:23.4: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:49:33.33 +55:08:08.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:49:33.33 +55:08:08.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:52:21.38 +51:55:18.8: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:52:21.38 +51:55:18.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:36:09.08 +55:02:17.9: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:43:12.87 +51:47:38.5: 12.65 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:36:09.08 +55:02:17.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:43:12.87 +51:47:38.5: 12.61 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.09
Forced photometry filter REJECTED candidate at 23:43:12.87 +51:47:38.5: ref_mag=12.64 +/- 0.09 new_mean_mag=12.0113 delta=0.63 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:04:35.68 +54:16:59.0: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:04:35.68 +54:16:59.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:32:07.88 +50:45:59.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:30:49.93 +57:02:05.0: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:30:49.93 +57:02:05.0: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:32:07.88 +50:45:59.5: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:47.02 +56:40:02.3: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:51.05 +56:07:30.1: 11.93 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:47.02 +56:40:02.3: 12.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:30:42.49 +51:34:34.0: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:51.05 +56:07:30.1: 11.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.04
Forced photometry filter REJECTED candidate at 23:51:51.05 +56:07:30.1: ref_mag=11.82 +/- 0.04 new_mean_mag=11.9004 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:30:42.49 +51:34:34.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:30:47.77 +57:05:47.3: 11.21 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:30:47.77 +57:05:47.3: 10.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.02
Forced photometry filter REJECTED candidate at 23:30:47.77 +57:05:47.3: ref_mag=11.09 +/- 0.02 new_mean_mag=12.1810 delta=-1.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:02:42.98 +50:56:43.9: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:02:42.98 +50:56:43.9: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:42:27.42 +53:50:34.9: 13.62 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:42:27.42 +53:50:34.9: 13.07 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.18
Forced photometry filter KEPT candidate at 23:42:27.42 +53:50:34.9: ref_mag=13.28 +/- 0.18 new_mean_mag=12.0282 delta=1.26 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:17.90 +57:21:29.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:17.90 +57:21:29.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:45:04.99 +50:54:58.6: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:45:04.99 +50:54:58.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:44:38.43 +57:28:10.9: 11.20 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:46:34.48 +57:42:57.7: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:19:47.50 +56:13:02.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:44:38.43 +57:28:10.9: 10.86 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.02
Forced photometry filter REJECTED candidate at 23:44:38.43 +57:28:10.9: ref_mag=11.03 +/- 0.02 new_mean_mag=11.8475 delta=-0.82 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:34.48 +57:42:57.7: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:19:47.50 +56:13:02.4: 13.05 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.28
Forced photometry filter KEPT candidate at 23:19:47.50 +56:13:02.4: ref_mag=13.05 +/- 0.28 new_mean_mag=11.6301 delta=1.42 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:11:44.35 +50:55:14.3: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:11:44.35 +50:55:14.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:00:46.08 +57:27:12.0: 11.67 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:00:46.08 +57:27:12.0: 11.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.04
Forced photometry filter REJECTED candidate at 00:00:46.08 +57:27:12.0: ref_mag=11.56 +/- 0.04 new_mean_mag=11.3843 delta=0.18 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:16.14 +53:25:17.0: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:07.04 +53:23:25.1: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:16.14 +53:25:17.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:07.04 +53:23:25.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:10:02.60 +56:51:39.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:22:56.28 +55:56:21.0: 13.29 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:10:02.60 +56:51:39.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:45:23.29 +53:48:02.7: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:22:56.28 +55:56:21.0: 13.37 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.18
Forced photometry filter KEPT candidate at 23:22:56.28 +55:56:21.0: ref_mag=13.31 +/- 0.18 new_mean_mag=11.4507 delta=1.86 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:45:23.29 +53:48:02.7: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:52.69 +57:46:42.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:52.69 +57:46:42.6: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:51:09.65 +55:30:06.1: 11.37 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:59:07.22 +54:42:32.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:51:09.65 +55:30:06.1: 11.06 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.03
Forced photometry filter KEPT candidate at 23:51:09.65 +55:30:06.1: ref_mag=11.21 +/- 0.03 new_mean_mag=9.9677 delta=1.25 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:59:07.22 +54:42:32.6: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:21:11.92 +50:00:10.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:04.93 +55:05:34.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:21:11.92 +50:00:10.5: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:04.93 +55:05:34.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:58:05.38 +56:28:01.2: 12.33 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:58:05.38 +56:28:01.2: 12.01 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.09
Forced photometry filter REJECTED candidate at 23:58:05.38 +56:28:01.2: ref_mag=12.17 +/- 0.09 new_mean_mag=11.4595 delta=0.71 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:17:56.55 +53:10:40.6: 10.72 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:17:56.55 +53:10:40.6: 10.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.02
Forced photometry filter REJECTED candidate at 23:17:56.55 +53:10:40.6: ref_mag=10.51 +/- 0.02 new_mean_mag=11.6674 delta=-1.16 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:56:52.64 +52:09:35.2: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:56:52.64 +52:09:35.2: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:19:31.89 +55:36:23.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:19:31.89 +55:36:23.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:33:40.95 +49:58:06.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:33:40.95 +49:58:06.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:35:43.42 +53:18:09.8: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:09:09.21 +49:47:10.2: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:35:43.42 +53:18:09.8: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:09:09.21 +49:47:10.2: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:14:42.28 +56:55:19.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:14:42.28 +56:55:19.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:09.68 +52:54:27.8: 13.63 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:14:47.95 +52:51:33.5: 13.48 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:09.68 +52:54:27.8: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:14:47.95 +52:51:33.5: 13.32 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.63 +/- 0.31
Forced photometry reference-image weighted average: 13.48 +/- 0.32
Forced photometry filter KEPT candidate at 23:14:47.95 +52:51:33.5: ref_mag=13.48 +/- 0.32 new_mean_mag=11.8960 delta=1.59 (need > 0.90)
Forced photometry filter KEPT candidate at 23:28:09.68 +52:54:27.8: ref_mag=13.63 +/- 0.31 new_mean_mag=11.9750 delta=1.66 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:13.86 +55:08:33.0: 12.13 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:13.86 +55:08:33.0: 11.79 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.05
Forced photometry filter REJECTED candidate at 23:57:13.86 +55:08:33.0: ref_mag=11.96 +/- 0.05 new_mean_mag=11.8614 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:48.89 +51:50:37.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:48.89 +51:50:37.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:20.99 +51:14:37.8: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:20.99 +51:14:37.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:00.77 +53:44:34.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:00.77 +53:44:34.5: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:52:04.12 +54:10:56.4: 11.71 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:52:04.12 +54:10:56.4: 11.36 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.03
Forced photometry filter REJECTED candidate at 23:52:04.12 +54:10:56.4: ref_mag=11.53 +/- 0.03 new_mean_mag=12.0676 delta=-0.54 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:33:49.55 +55:18:17.4: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:33:49.55 +55:18:17.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:11:59.48 +56:58:23.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:11:59.48 +56:58:23.3: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:05.53 +57:36:00.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:05.53 +57:36:00.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:10:53.96 +56:47:38.6: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:10:53.96 +56:47:38.6: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:24:08.33 +56:51:15.0: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:24:08.33 +56:51:15.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:59.04 +51:16:49.6: 13.51 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:33:04.47 +54:43:12.4: 13.05 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:59.04 +51:16:49.6: 13.49 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.51 +/- 0.29
Forced photometry filter KEPT candidate at 23:25:59.04 +51:16:49.6: ref_mag=13.51 +/- 0.29 new_mean_mag=12.4002 delta=1.11 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:33:04.47 +54:43:12.4: 13.47 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.05 +/- 0.19
Forced photometry filter REJECTED candidate at 23:33:04.47 +54:43:12.4: ref_mag=13.05 +/- 0.19 new_mean_mag=12.3659 delta=0.69 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:07:17.52 +58:04:10.9: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:17.52 +58:04:10.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:21:02.63 +55:32:43.1: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:21:02.63 +55:32:43.1: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:31:47.05 +52:31:41.9: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:31:47.05 +52:31:41.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:04.90 +57:12:06.6: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:04.90 +57:12:06.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:20:53.67 +56:39:59.8: 13.59 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:20:53.67 +56:39:59.8: 13.43 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.59 +/- 0.33
Forced photometry filter KEPT candidate at 23:20:53.67 +56:39:59.8: ref_mag=13.59 +/- 0.33 new_mean_mag=12.6245 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:13:34.42 +55:35:38.4: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:13:34.42 +55:35:38.4: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:17:02.07 +54:44:50.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:32:53.70 +54:41:15.1: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:17:02.07 +54:44:50.6: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:32:53.70 +54:41:15.1: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:21.92 +58:13:32.3: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:21.92 +58:13:32.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:55:53.24 +57:04:30.3: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:55:55.87 +56:01:47.1: 13.13 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:55:53.24 +57:04:30.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:55:55.87 +56:01:47.1: 12.76 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.13
Forced photometry filter REJECTED candidate at 23:55:55.87 +56:01:47.1: ref_mag=12.93 +/- 0.13 new_mean_mag=12.6334 delta=0.30 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:37:17.75 +53:04:18.5: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:37:17.75 +53:04:18.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:14:09.17 +57:57:33.4: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:57.42 +56:07:12.8: 13.08 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:14:09.17 +57:57:33.4: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:54:57.42 +56:07:12.8: 12.81 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.13
Forced photometry filter REJECTED candidate at 23:54:57.42 +56:07:12.8: ref_mag=12.95 +/- 0.13 new_mean_mag=12.5933 delta=0.36 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:49:01.53 +56:53:05.0: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:49:01.53 +56:53:05.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:19.10 +53:25:13.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:19.10 +53:25:13.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:44:55.96 +55:59:33.2: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:44:55.96 +55:59:33.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:02:10.03 +57:51:20.3: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:02:10.03 +57:51:20.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:58.83 +55:53:58.1: 12.73 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:54:58.83 +55:53:58.1: 12.63 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.10
Forced photometry filter REJECTED candidate at 23:54:58.83 +55:53:58.1: ref_mag=12.69 +/- 0.10 new_mean_mag=12.7431 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:46:41.19 +54:17:34.0: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:41.19 +54:17:34.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:21:08.08 +55:12:51.0: 13.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:21:08.08 +55:12:51.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:05:58.74 +53:50:18.5: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:05:58.74 +53:50:18.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:54.71 +54:18:51.1: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:54.71 +54:18:51.1: 13.45 +/- 99.00 upperlimit
Adding exclusion_list_gaiadr2.txt__out190495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out189857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87727.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 139s
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: 80s
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Considering the candidate 189817_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189817_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (28.2") between the two second-epoch detections
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Considering the candidate 189857_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189857_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189874_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189874_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189875_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189875_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189885_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189885_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 189888_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189888_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189889_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189889_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 189900_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189900_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189902_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189902_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 189904_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189904_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189907_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189907_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 189908_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189908_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 189909_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189909_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189918_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189918_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189925_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189925_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189937_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189937_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189939_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189939_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189948_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189948_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189954_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189954_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189970_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189970_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 189980_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189980_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189982_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189982_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 189984_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189984_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189986_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189986_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189988_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189988_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:15:53.33 +52:29:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189992_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 189992_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:48:17.74 +53:25:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189994_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189994_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189995_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189995_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 189996_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 189996_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190006_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190006_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190011_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190011_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190015_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190015_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190016_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190016_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190022_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190022_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:29:32.91 +53:51:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190024_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190024_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190034_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190034_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190035_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190035_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190036_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190036_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190040_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190040_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190047_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190047_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:08:36.97 +55:38:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190049_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190049_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190051_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190051_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190056_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190056_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190057_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190057_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190060_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190060_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190062_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190062_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190063_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190063_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190071_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190071_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190073_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190073_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190078_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190078_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190079_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190079_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190083_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190083_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:54:22.09 +55:10:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190087_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190087_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 190089_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190089_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:25:16.32 +53:39:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190096_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190096_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:12:59.72 +54:44:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190104_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190104_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:04:21.93 +51:49:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190111_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190111_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:48:19.64 +54:50:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190113_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190113_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190115_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190115_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190116_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190116_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190120_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190120_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190121_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190121_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:26:42.66 +54:33:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190122_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190122_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190124_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190124_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:26:29.44 +57:34:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190126_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190126_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190128_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190128_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190129_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190129_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:23:06.49 +53:52:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190135_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190135_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:20:25.35 +53:17:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190136_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190136_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:45:59.18 +56:53:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190140_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190140_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190148_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190148_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190153_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190153_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190154_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190154_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:14:23.66 +54:44:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190156_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190156_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:21:35.26 +50:17:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190157_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190157_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190159_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190159_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:29:03.42 +55:22:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190162_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190162_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:21:54.32 +51:47:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190172_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190172_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:28:10.95 +56:29:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190173_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190173_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 190177_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190177_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190317_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190317_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190371_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190371_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:59:23.85 +50:31:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190403_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190403_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:18:49.85 +54:33:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190409_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190409_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:23:03.57 +55:45:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190451_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190451_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:12:28.19 +57:05:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190464_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190464_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:25:37.27 +53:21:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190478_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190478_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:12:53.38 +57:44:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190495_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190495_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:21:11.92 +50:00:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 3.473 1991161548689209984 350.29831220230 +50.00333248370 9.7912 8.5016 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 190502_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190502_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190510_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190510_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:19:32.89 +57:40:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190533_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190533_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190541_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190541_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:57:59.54 +50:26:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190569_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190569_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190597_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190597_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190615_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190615_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190617_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190617_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190624_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190624_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:28:20.89 +54:48:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190630_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190630_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:35:18.81 +50:19:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190635_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190635_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:10:09.16 +58:07:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190654_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190654_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190660_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190660_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190666_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190666_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:52:36.18 +50:18:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190668_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190668_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:10:28.94 +49:51:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190680_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190680_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:08:02.07 +53:40:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190682_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190682_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:32:51.55 +51:53:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190689_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190689_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190694_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190694_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:20:56.36 +56:24:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190706_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190706_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190714_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190714_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190715_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190715_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:27:11.43 +53:53:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190717_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190717_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:04:15.13 +54:16:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190742_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190742_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190743_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190743_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:03:01.83 +50:28:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190750_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190750_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:29:46.77 +54:39:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190755_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190755_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:52:01.70 +50:05:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190759_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190759_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190782_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190782_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:31:16.91 +57:14:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190789_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190789_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:01:49.64 +52:51:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190790_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190790_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:12:20.42 +50:38:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190797_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190797_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190812_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190812_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:22:24.17 +54:06:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190814_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190814_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190850_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190850_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:00:26.38 +55:27:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190853_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190853_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190864_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190864_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:54:44.64 +53:43:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190875_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190875_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190876_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190876_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190899_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190899_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190913_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190913_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190918_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190918_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190931_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190931_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:54:31.64 +54:58:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190939_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190939_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190946_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 190946_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 190961_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190961_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190987_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190987_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 190995_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 190995_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 191006_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191006_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191031_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 191031_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:07:40.71 +57:11:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191066_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191066_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 191080_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191080_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 191082_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191082_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191090_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191090_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191093_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191093_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191105_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191105_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 191126_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 191126_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
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Considering the candidate 191158_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191158_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191162_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191162_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191169_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 191169_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191175_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191175_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191178_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191178_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 191181_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191181_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
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Considering the candidate 191199_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191199_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191207_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 191207_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191221_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191221_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191239_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191239_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191284_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 191284_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140320_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 140320_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:44:31.90 +56:34:49.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139426_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 139426_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 23:11:31.20 +56:01:28.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87727_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
Preparing report for the candidate 87727_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179849_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 179849_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:15:50.73 +57:32:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35911_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 35911_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:09:36.46 +51:34:01.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75760_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 75760_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:26:05.85 +53:55:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105722_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071
The candidate 105722_fd_Cas-04-Q2b1x1_2026-07-13_23-03-32_20.00sec_5.00C_LIGHT_0071 did not pass the final checks
**** FOUND 00:04:40.68 +55:32:13.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 225s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:51:09.70 +53:46:57.8
23:56:12.73 +54:27:13.9
23:58:03.04 +56:41:42.7
00:21:25.15 +52:13:59.1
23:43:42.88 +53:55:36.1
23:24:16.99 +54:08:47.4
23:17:09.99 +56:15:31.3
23:53:10.35 +53:59:59.2
00:23:31.51 +57:49:05.2
23:43:39.23 +56:09:51.3
23:58:11.78 +57:33:41.6
23:37:18.44 +52:28:49.3
23:55:59.53 +54:35:43.1
23:50:53.38 +53:45:32.0
23:35:48.73 +53:57:55.9
00:03:11.56 +53:21:29.4
23:45:22.60 +56:43:43.9
00:17:55.26 +57:40:39.0
23:32:17.21 +53:33:23.2
23:42:19.55 +53:35:56.3
23:51:53.10 +53:41:36.0
23:29:13.57 +52:52:54.0
23:43:42.98 +55:12:23.4
23:49:33.33 +55:08:08.6
23:52:21.38 +51:55:18.8
23:36:09.08 +55:02:17.9
00:04:35.68 +54:16:59.0
23:30:49.93 +57:02:05.0
23:32:07.88 +50:45:59.5
23:57:47.02 +56:40:02.3
23:30:42.49 +51:34:34.0
00:02:42.98 +50:56:43.9
23:42:27.42 +53:50:34.9
00:07:17.90 +57:21:29.9
23:45:04.99 +50:54:58.6
23:46:34.48 +57:42:57.7
23:19:47.50 +56:13:02.4
00:11:44.35 +50:55:14.3
23:51:16.14 +53:25:17.0
00:27:07.04 +53:23:25.1
23:22:56.28 +55:56:21.0
23:10:02.60 +56:51:39.6
23:45:23.29 +53:48:02.7
00:17:52.69 +57:46:42.6
23:51:09.65 +55:30:06.1
23:59:07.22 +54:42:32.6
23:25:04.93 +55:05:34.5
23:56:52.64 +52:09:35.2
23:19:31.89 +55:36:23.6
23:33:40.95 +49:58:06.8
23:35:43.42 +53:18:09.8
00:09:09.21 +49:47:10.2
23:14:42.28 +56:55:19.2
23:28:09.68 +52:54:27.8
23:14:47.95 +52:51:33.5
23:25:48.89 +51:50:37.5
23:29:20.99 +51:14:37.8
23:57:00.77 +53:44:34.5
23:33:49.55 +55:18:17.4
23:11:59.48 +56:58:23.3
00:28:05.53 +57:36:00.0
23:10:53.96 +56:47:38.6
23:24:08.33 +56:51:15.0
23:25:59.04 +51:16:49.6
00:07:17.52 +58:04:10.9
23:21:02.63 +55:32:43.1
23:31:47.05 +52:31:41.9
23:25:04.90 +57:12:06.6
23:20:53.67 +56:39:59.8
23:13:34.42 +55:35:38.4
23:17:02.07 +54:44:50.6
23:32:53.70 +54:41:15.1
00:17:21.92 +58:13:32.3
23:55:53.24 +57:04:30.3
23:37:17.75 +53:04:18.5
00:14:09.17 +57:57:33.4
23:49:01.53 +56:53:05.0
23:29:19.10 +53:25:13.0
23:44:55.96 +55:59:33.2
00:02:10.03 +57:51:20.3
23:46:41.19 +54:17:34.0
00:21:08.08 +55:12:51.0
00:05:58.74 +53:50:18.5
23:28:54.71 +54:18:51.1
########### Completed Cas-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
23:51:09.70 +53:46:57.8
23:56:12.73 +54:27:13.9
23:58:03.04 +56:41:42.7
00:21:25.15 +52:13:59.1
23:43:42.88 +53:55:36.1
23:24:16.99 +54:08:47.4
23:17:09.99 +56:15:31.3
23:53:10.35 +53:59:59.2
00:23:31.51 +57:49:05.2
23:43:39.23 +56:09:51.3
23:58:11.78 +57:33:41.6
23:37:18.44 +52:28:49.3
23:55:59.53 +54:35:43.1
23:50:53.38 +53:45:32.0
23:35:48.73 +53:57:55.9
00:03:11.56 +53:21:29.4
23:45:22.60 +56:43:43.9
00:17:55.26 +57:40:39.0
23:32:17.21 +53:33:23.2
23:42:19.55 +53:35:56.3
23:51:53.10 +53:41:36.0
23:29:13.57 +52:52:54.0
23:43:42.98 +55:12:23.4
23:49:33.33 +55:08:08.6
23:52:21.38 +51:55:18.8
23:36:09.08 +55:02:17.9
00:04:35.68 +54:16:59.0
23:30:49.93 +57:02:05.0
23:32:07.88 +50:45:59.5
23:57:47.02 +56:40:02.3
23:30:42.49 +51:34:34.0
00:02:42.98 +50:56:43.9
23:42:27.42 +53:50:34.9
00:07:17.90 +57:21:29.9
23:45:04.99 +50:54:58.6
23:46:34.48 +57:42:57.7
23:19:47.50 +56:13:02.4
00:11:44.35 +50:55:14.3
23:51:16.14 +53:25:17.0
00:27:07.04 +53:23:25.1
23:22:56.28 +55:56:21.0
23:10:02.60 +56:51:39.6
23:45:23.29 +53:48:02.7
00:17:52.69 +57:46:42.6
23:51:09.65 +55:30:06.1
23:59:07.22 +54:42:32.6
23:25:04.93 +55:05:34.5
23:56:52.64 +52:09:35.2
23:19:31.89 +55:36:23.6
23:33:40.95 +49:58:06.8
23:35:43.42 +53:18:09.8
00:09:09.21 +49:47:10.2
23:14:42.28 +56:55:19.2
23:28:09.68 +52:54:27.8
23:14:47.95 +52:51:33.5
23:25:48.89 +51:50:37.5
23:29:20.99 +51:14:37.8
23:57:00.77 +53:44:34.5
23:33:49.55 +55:18:17.4
23:11:59.48 +56:58:23.3
00:28:05.53 +57:36:00.0
23:10:53.96 +56:47:38.6
23:24:08.33 +56:51:15.0
23:25:59.04 +51:16:49.6
00:07:17.52 +58:04:10.9
23:21:02.63 +55:32:43.1
23:31:47.05 +52:31:41.9
23:25:04.90 +57:12:06.6
23:20:53.67 +56:39:59.8
23:13:34.42 +55:35:38.4
23:17:02.07 +54:44:50.6
23:32:53.70 +54:41:15.1
00:17:21.92 +58:13:32.3
23:55:53.24 +57:04:30.3
23:37:17.75 +53:04:18.5
00:14:09.17 +57:57:33.4
23:49:01.53 +56:53:05.0
23:29:19.10 +53:25:13.0
23:44:55.96 +55:59:33.2
00:02:10.03 +57:51:20.3
23:46:41.19 +54:17:34.0
00:21:08.08 +55:12:51.0
00:05:58.74 +53:50:18.5
23:28:54.71 +54:18:51.1
###################################################################################
23:51:09.70 +53:46:57.8 -- not an asteroid (will add it to exclusion list)
23:56:12.73 +54:27:13.9 -- not an asteroid (will add it to exclusion list)
23:58:03.04 +56:41:42.7 -- not an asteroid (will add it to exclusion list)
00:21:25.15 +52:13:59.1 -- not an asteroid (will add it to exclusion list)
23:43:42.88 +53:55:36.1 -- not an asteroid (will add it to exclusion list)
23:24:16.99 +54:08:47.4 -- not an asteroid (will add it to exclusion list)
23:17:09.99 +56:15:31.3 -- not an asteroid (will add it to exclusion list)
23:53:10.35 +53:59:59.2 -- not an asteroid (will add it to exclusion list)
00:23:31.51 +57:49:05.2 -- not an asteroid (will add it to exclusion list)
23:43:39.23 +56:09:51.3 -- not an asteroid (will add it to exclusion list)
23:58:11.78 +57:33:41.6 -- not an asteroid (will add it to exclusion list)
23:37:18.44 +52:28:49.3 -- not an asteroid (will add it to exclusion list)
23:55:59.53 +54:35:43.1 -- not an asteroid (will add it to exclusion list)
23:50:53.38 +53:45:32.0 -- not an asteroid (will add it to exclusion list)
23:35:48.73 +53:57:55.9 -- not an asteroid (will add it to exclusion list)
00:03:11.56 +53:21:29.4 -- not an asteroid (will add it to exclusion list)
23:45:22.60 +56:43:43.9 -- not an asteroid (will add it to exclusion list)
00:17:55.26 +57:40:39.0 -- not an asteroid (will add it to exclusion list)
23:32:17.21 +53:33:23.2 -- not an asteroid (will add it to exclusion list)
23:42:19.55 +53:35:56.3 -- not an asteroid (will add it to exclusion list)
23:51:53.10 +53:41:36.0 -- not an asteroid (will add it to exclusion list)
23:29:13.57 +52:52:54.0 -- not an asteroid (will add it to exclusion list)
23:43:42.98 +55:12:23.4 -- not an asteroid (will add it to exclusion list)
23:49:33.33 +55:08:08.6 -- not an asteroid (will add it to exclusion list)
23:52:21.38 +51:55:18.8 -- not an asteroid (will add it to exclusion list)
23:36:09.08 +55:02:17.9 -- not an asteroid (will add it to exclusion list)
00:04:35.68 +54:16:59.0 -- not an asteroid (will add it to exclusion list)
23:30:49.93 +57:02:05.0 -- not an asteroid (will add it to exclusion list)
23:32:07.88 +50:45:59.5 -- not an asteroid (will add it to exclusion list)
23:57:47.02 +56:40:02.3 -- not an asteroid (will add it to exclusion list)
23:30:42.49 +51:34:34.0 -- not an asteroid (will add it to exclusion list)
00:02:42.98 +50:56:43.9 -- not an asteroid (will add it to exclusion list)
23:42:27.42 +53:50:34.9 -- not an asteroid (will add it to exclusion list)
00:07:17.90 +57:21:29.9 -- not an asteroid (will add it to exclusion list)
23:45:04.99 +50:54:58.6 -- not an asteroid (will add it to exclusion list)
23:46:34.48 +57:42:57.7 -- not an asteroid (will add it to exclusion list)
23:19:47.50 +56:13:02.4 -- not an asteroid (will add it to exclusion list)
00:11:44.35 +50:55:14.3 -- not an asteroid (will add it to exclusion list)
23:51:16.14 +53:25:17.0 -- not an asteroid (will add it to exclusion list)
00:27:07.04 +53:23:25.1 -- not an asteroid (will add it to exclusion list)
23:22:56.28 +55:56:21.0 -- not an asteroid (will add it to exclusion list)
23:10:02.60 +56:51:39.6 -- not an asteroid (will add it to exclusion list)
23:45:23.29 +53:48:02.7 -- not an asteroid (will add it to exclusion list)
00:17:52.69 +57:46:42.6 -- not an asteroid (will add it to exclusion list)
23:51:09.65 +55:30:06.1 -- not an asteroid (will add it to exclusion list)
23:59:07.22 +54:42:32.6 -- not an asteroid (will add it to exclusion list)
23:25:04.93 +55:05:34.5 -- not an asteroid (will add it to exclusion list)
23:56:52.64 +52:09:35.2 -- not an asteroid (will add it to exclusion list)
23:19:31.89 +55:36:23.6 -- not an asteroid (will add it to exclusion list)
23:33:40.95 +49:58:06.8 -- not an asteroid (will add it to exclusion list)
23:35:43.42 +53:18:09.8 -- not an asteroid (will add it to exclusion list)
00:09:09.21 +49:47:10.2 -- not an asteroid (will add it to exclusion list)
23:14:42.28 +56:55:19.2 -- not an asteroid (will add it to exclusion list)
23:28:09.68 +52:54:27.8 -- not an asteroid (will add it to exclusion list)
23:14:47.95 +52:51:33.5 -- not an asteroid (will add it to exclusion list)
23:25:48.89 +51:50:37.5 -- not an asteroid (will add it to exclusion list)
23:29:20.99 +51:14:37.8 -- not an asteroid (will add it to exclusion list)
23:57:00.77 +53:44:34.5 -- not an asteroid (will add it to exclusion list)
23:33:49.55 +55:18:17.4 -- not an asteroid (will add it to exclusion list)
23:11:59.48 +56:58:23.3 -- not an asteroid (will add it to exclusion list)
00:28:05.53 +57:36:00.0 -- not an asteroid (will add it to exclusion list)
23:10:53.96 +56:47:38.6 -- not an asteroid (will add it to exclusion list)
23:24:08.33 +56:51:15.0 -- not an asteroid (will add it to exclusion list)
23:25:59.04 +51:16:49.6 -- not an asteroid (will add it to exclusion list)
00:07:17.52 +58:04:10.9 -- not an asteroid (will add it to exclusion list)
23:21:02.63 +55:32:43.1 -- not an asteroid (will add it to exclusion list)
23:31:47.05 +52:31:41.9 -- not an asteroid (will add it to exclusion list)
23:25:04.90 +57:12:06.6 -- not an asteroid (will add it to exclusion list)
23:20:53.67 +56:39:59.8 -- not an asteroid (will add it to exclusion list)
23:13:34.42 +55:35:38.4 -- not an asteroid (will add it to exclusion list)
23:17:02.07 +54:44:50.6 -- not an asteroid (will add it to exclusion list)
23:32:53.70 +54:41:15.1 -- not an asteroid (will add it to exclusion list)
00:17:21.92 +58:13:32.3 -- not an asteroid (will add it to exclusion list)
23:55:53.24 +57:04:30.3 -- not an asteroid (will add it to exclusion list)
23:37:17.75 +53:04:18.5 -- not an asteroid (will add it to exclusion list)
00:14:09.17 +57:57:33.4 -- not an asteroid (will add it to exclusion list)
23:49:01.53 +56:53:05.0 -- not an asteroid (will add it to exclusion list)
23:29:19.10 +53:25:13.0 -- not an asteroid (will add it to exclusion list)
23:44:55.96 +55:59:33.2 -- not an asteroid (will add it to exclusion list)
00:02:10.03 +57:51:20.3 -- not an asteroid (will add it to exclusion list)
23:46:41.19 +54:17:34.0 -- not an asteroid (will add it to exclusion list)
00:21:08.08 +55:12:51.0 -- not an asteroid (will add it to exclusion list)
00:05:58.74 +53:50:18.5 -- not an asteroid (will add it to exclusion list)
23:28:54.71 +54:18:51.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:02:10.03 +57:51:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:42.98 +50:56:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:11.56 +53:21:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:35.68 +54:16:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:58.74 +53:50:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:17.52 +58:04:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:17.90 +57:21:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:09.21 +49:47:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:44.35 +50:55:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:09.17 +57:57:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:21.92 +58:13:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:52.69 +57:46:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:55.26 +57:40:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:08.08 +55:12:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:25.15 +52:13:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:31.51 +57:49:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:07.04 +53:23:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:05.53 +57:36:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:02.60 +56:51:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:53.96 +56:47:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:59.48 +56:58:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:34.42 +55:35:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:42.28 +56:55:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:47.95 +52:51:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:02.07 +54:44:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:09.99 +56:15:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:31.89 +55:36:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:47.50 +56:13:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:53.67 +56:39:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:02.63 +55:32:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:56.28 +55:56:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:08.33 +56:51:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:16.99 +54:08:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:04.90 +57:12:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:04.93 +55:05:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:48.89 +51:50:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:59.04 +51:16:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:09.68 +52:54:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:54.71 +54:18:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:13.57 +52:52:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:19.10 +53:25:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:20.99 +51:14:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:42.49 +51:34:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:49.93 +57:02:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:47.05 +52:31:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:07.88 +50:45:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:17.21 +53:33:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:53.70 +54:41:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:40.95 +49:58:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:49.55 +55:18:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:43.42 +53:18:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:48.73 +53:57:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:09.08 +55:02:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:17.75 +53:04:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:18.44 +52:28:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:19.55 +53:35:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:27.42 +53:50:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:39.23 +56:09:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:42.88 +53:55:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:42.98 +55:12:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:55.96 +55:59:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:04.99 +50:54:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:22.60 +56:43:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:23.29 +53:48:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:34.48 +57:42:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:41.19 +54:17:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:01.53 +56:53:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:33.33 +55:08:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:53.38 +53:45:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:09.65 +55:30:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:09.70 +53:46:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:16.14 +53:25:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:53.10 +53:41:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:21.38 +51:55:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:10.35 +53:59:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:53.24 +57:04:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:59.53 +54:35:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:12.73 +54:27:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:52.64 +52:09:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:00.77 +53:44:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:47.02 +56:40:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:03.04 +56:41:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:11.78 +57:33:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:07.22 +54:42:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:02:10.03 +57:51:20.3 -- not a known variable star
00:02:42.98 +50:56:43.9 -- a known variable star
00:03:11.56 +53:21:29.4 -- not a known variable star
00:04:35.68 +54:16:59.0 -- not a known variable star
00:05:58.74 +53:50:18.5 -- not a known variable star
00:07:17.52 +58:04:10.9 -- not a known variable star
00:07:17.90 +57:21:29.9 -- not a known variable star
00:09:09.21 +49:47:10.2 -- not a known variable star
00:11:44.35 +50:55:14.3 -- a known variable star
00:14:09.17 +57:57:33.4 -- not a known variable star
00:17:21.92 +58:13:32.3 -- not a known variable star
00:17:52.69 +57:46:42.6 -- not a known variable star
00:17:55.26 +57:40:39.0 -- not a known variable star
00:21:08.08 +55:12:51.0 -- not a known variable star
00:21:25.15 +52:13:59.1 -- not a known variable star
00:23:31.51 +57:49:05.2 -- a known variable star
00:27:07.04 +53:23:25.1 -- not a known variable star
00:28:05.53 +57:36:00.0 -- not a known variable star
23:10:02.60 +56:51:39.6 -- not a known variable star
23:10:53.96 +56:47:38.6 -- not a known variable star
23:11:59.48 +56:58:23.3 -- not a known variable star
23:13:34.42 +55:35:38.4 -- a known variable star
23:14:42.28 +56:55:19.2 -- not a known variable star
23:14:47.95 +52:51:33.5 -- a known variable star
23:17:02.07 +54:44:50.6 -- a known variable star
23:17:09.99 +56:15:31.3 -- not a known variable star
23:19:31.89 +55:36:23.6 -- not a known variable star
23:19:47.50 +56:13:02.4 -- not a known variable star
23:20:53.67 +56:39:59.8 -- not a known variable star
23:21:02.63 +55:32:43.1 -- not a known variable star
23:22:56.28 +55:56:21.0 -- not a known variable star
23:24:08.33 +56:51:15.0 -- not a known variable star
23:24:16.99 +54:08:47.4 -- not a known variable star
23:25:04.90 +57:12:06.6 -- not a known variable star
23:25:04.93 +55:05:34.5 -- not a known variable star
23:25:48.89 +51:50:37.5 -- not a known variable star
23:25:59.04 +51:16:49.6 -- not a known variable star
23:28:09.68 +52:54:27.8 -- not a known variable star
23:28:54.71 +54:18:51.1 -- not a known variable star
23:29:13.57 +52:52:54.0 -- a known variable star
23:29:19.10 +53:25:13.0 -- not a known variable star
23:29:20.99 +51:14:37.8 -- not a known variable star
23:30:42.49 +51:34:34.0 -- a known variable star
23:30:49.93 +57:02:05.0 -- not a known variable star
23:31:47.05 +52:31:41.9 -- not a known variable star
23:32:07.88 +50:45:59.5 -- not a known variable star
23:32:17.21 +53:33:23.2 -- not a known variable star
23:32:53.70 +54:41:15.1 -- not a known variable star
23:33:40.95 +49:58:06.8 -- not a known variable star
23:33:49.55 +55:18:17.4 -- a known variable star
23:35:43.42 +53:18:09.8 -- not a known variable star
23:35:48.73 +53:57:55.9 -- a known variable star
23:36:09.08 +55:02:17.9 -- not a known variable star
23:37:17.75 +53:04:18.5 -- a known variable star
23:37:18.44 +52:28:49.3 -- not a known variable star
23:42:19.55 +53:35:56.3 -- not a known variable star
23:42:27.42 +53:50:34.9 -- a known variable star
23:43:39.23 +56:09:51.3 -- not a known variable star
23:43:42.88 +53:55:36.1 -- not a known variable star
23:43:42.98 +55:12:23.4 -- not a known variable star
23:44:55.96 +55:59:33.2 -- not a known variable star
23:45:04.99 +50:54:58.6 -- not a known variable star
23:45:22.60 +56:43:43.9 -- not a known variable star
23:45:23.29 +53:48:02.7 -- not a known variable star
23:46:34.48 +57:42:57.7 -- not a known variable star
23:46:41.19 +54:17:34.0 -- not a known variable star
23:49:01.53 +56:53:05.0 -- not a known variable star
23:49:33.33 +55:08:08.6 -- not a known variable star
23:50:53.38 +53:45:32.0 -- not a known variable star
23:51:09.65 +55:30:06.1 -- not a known variable star
23:51:09.70 +53:46:57.8 -- a known variable star
23:51:16.14 +53:25:17.0 -- a known variable star
23:51:53.10 +53:41:36.0 -- not a known variable star
23:52:21.38 +51:55:18.8 -- not a known variable star
23:53:10.35 +53:59:59.2 -- not a known variable star
23:55:53.24 +57:04:30.3 -- not a known variable star
23:55:59.53 +54:35:43.1 -- not a known variable star
23:56:12.73 +54:27:13.9 -- a known variable star
23:56:52.64 +52:09:35.2 -- not a known variable star
23:57:00.77 +53:44:34.5 -- not a known variable star
23:57:47.02 +56:40:02.3 -- not a known variable star
23:58:03.04 +56:41:42.7 -- not a known variable star
23:58:11.78 +57:33:41.6 -- not a known variable star
23:59:07.22 +54:42:32.6 -- not a known variable star
Found 69 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
84 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 84 (excluding asteroids and hot pixels, 69 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)2461235.66869972 -observatory V36
07:21:58.84 +17:08:53.2 Mercury (5.5mag)
10:27:28.60 +10:58:54.0 Venus (-4.1mag)
04:35:29.31 +21:52:25.9 Mars (1.3mag)
08:20:08.88 +20:00:25.1 Jupiter (-1.8mag)
00:56:13.43 +03:21:40.9 Saturn (0.7mag)
04:07:56.97 +20:46:59.1 Uranus (5.8mag)
00:16:59.59 +00:20:15.8 Neptune (7.7mag)
20:30:33.68 -23:19:41.4 Pluto (14.4mag)
07:17:46.64 +24:52:39.0 Moon (99.9mag)
-rw-r--r-- 1 apache apache 361 Jul 14 00:21 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461235.66869972:
08:20:16.14 +19:59:57.7 Io (6.1mag)
08:20:15.96 +19:59:59.6 Europa (6.3mag)
08:19:54.19 +20:01:21.3 Ganymede (5.6mag)
08:20:03.71 +20:00:40.2 Callisto (6.8mag)
08:18:30.02 +19:46:13.3 Himalia (15.7mag)
08:20:09.22 +20:00:24.6 Thebe (16.6mag)
08:17:50.75 +19:49:50.4 Elara (17.7mag)
08:23:48.00 +19:52:32.7 Pasiphae (17.8mag)
08:24:53.56 +20:06:03.6 Carme (19.0mag)
00:56:19.52 +03:21:10.8 Titan (8.5mag)
00:56:10.37 +03:21:51.7 Rhea (9.8mag)
00:55:39.30 +03:20:07.8 Iapetus (11.2mag)
00:56:06.11 +03:22:08.4 Hyperion (14.5mag)
00:56:09.06 +03:18:21.2 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 14 00:21 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461235.66869972:
17:52:16.33 -32:08:54.9 JWST
18:40:00.91 +23:14:16.6 Chandra
19:27:54.30 +04:46:08.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 14 00:21 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461235.66869972 -observatory V36
02:41:39.65 +14:52:38.2 17.9mag P/1996 R2 (Lagerkvist)
18:15:03.59 -34:27:42.1 13.8mag P/2010 H2 (Vales)
06:29:29.45 -68:12:13.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:02:07.46 +32:30:44.6 17.6mag C/2017 K2 (PANSTARRS)
02:08:30.75 +15:12:33.0 15.6mag P/2021 N1 (ZTF)
22:57:11.63 +32:16:14.3 17.3mag C/2022 E2 (ATLAS)
06:16:44.31 +26:53:27.4 16.7mag C/2022 N2 (PANSTARRS)
09:58:51.10 +29:36:35.5 16.9mag C/2022 QE78 (ATLAS)
09:12:12.36 +05:04:09.6 17.8mag C/2022 R6 (PANSTARRS)
18:04:55.19 +21:08:26.9 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:15.18 -11:28:40.7 17.7mag P/2023 B1 (PANSTARRS)
21:44:33.67 +67:34:51.8 17.8mag C/2023 H5 (Lemmon)
16:23:31.99 -10:28:33.7 13.9mag C/2023 R1 (PANSTARRS)
08:07:18.42 +65:54:58.5 17.9mag C/2024 A1 (ATLAS)
07:37:47.34 +30:11:45.6 14.7mag C/2024 E1 (Wierzchos)
15:14:32.35 +15:25:20.7 17.6mag C/2024 G6 (ATLAS)
19:36:24.58 +40:06:58.4 13.8mag C/2024 J3 (ATLAS)
21:43:32.75 +46:34:00.4 17.8mag C/2024 R4 (PANSTARRS)
04:53:13.64 -13:37:42.6 15.7mag C/2024 T5 (ATLAS)
06:37:42.88 +28:25:58.8 18.0mag C/2025 J1 (Borisov)
07:16:58.48 -13:14:06.8 16.7mag C/2025 R3 (PANSTARRS)
10:00:33.38 +22:16:12.4 17.6mag C/2025 V2 (Rankin)
12:45:56.40 +03:46:13.8 17.1mag C/2025 Y1 (ATLAS)
16:41:24.96 +79:10:06.5 17.3mag C/2026 A2 (Bok)
02:50:13.89 +45:24:07.8 16.7mag C/2026 B2 (Sun-Gao)
11:27:58.74 +05:12:26.2 17.0mag A/2026 E1
21:24:59.86 -16:28:43.6 7.2mag 10P/Tempel
11:15:16.13 -02:03:13.1 16.2mag 29P/Schwassmann-Wachmann
04:05:39.30 +29:57:56.2 17.9mag 47P/Ashbrook-Jackson
10:16:02.67 +12:47:33.7 17.1mag 63P/Wild
00:49:56.97 -05:03:24.3 15.5mag 65P/Gunn
04:36:37.38 +20:21:57.1 13.7mag 78P/Gehrels
02:28:26.12 +11:07:37.7 16.3mag 88P/Howell
06:46:50.85 +30:17:41.4 15.7mag 93P/Lovas
04:33:25.44 +31:15:38.6 16.8mag 114P/Wiseman-Skiff
08:18:01.36 +30:16:09.7 15.2mag 123P/West-Hartley
10:55:16.05 -00:21:50.6 16.8mag 124P/Mrkos
04:57:51.10 +20:55:02.5 16.2mag 128P/Shoemaker-Holt
05:43:26.43 +19:40:39.3 17.8mag 131P/Mueller
00:02:31.07 +03:04:39.5 17.9mag 139P/Vaisala-Oterma
07:27:27.47 +16:11:10.4 16.0mag 141P-D/Machholz
03:18:23.66 -20:47:39.3 15.3mag 161P/Hartley-IRAS
05:46:49.38 +34:44:35.6 15.4mag 162P/SidingSpring
18:53:54.09 +17:31:32.9 14.4mag 169P/NEAT
01:50:05.47 +08:00:51.6 17.7mag 220P/McNaught
16:35:34.33 -08:32:39.2 17.1mag 235P/LINEAR
08:53:18.70 +32:56:34.5 18.0mag 240P/NEAT
20:40:24.13 -50:22:47.9 17.8mag 259P/Garradd
02:10:00.94 +13:52:48.9 15.6mag 260P/McNaught
05:48:49.45 +37:07:59.6 17.4mag 295P/LINEAR
15:06:28.77 +05:42:45.2 17.6mag 391P/Kowalski
08:38:02.22 +19:31:13.6 17.9mag 450P/LONEOS
07:57:45.03 +38:53:53.8 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 14 00:21 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 14 00:21 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
-rw-r--r-- 1 apache apache 189K Jul 14 00:21 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:28:03.757 -02:04:50.07 AT 2026ttz 2026-07-09.34 21.7676
22:28:44.738 -02:46:18.12 AT 2026tty 2026-07-09.34 22.9915
22:20:46.753 -10:45:21.00 AT 2026ttx 2026-07-07.39 22.4769
22:14:51.717 -14:51:45.88 AT 2026ttw 2026-07-07.42 22.8608
21:49:49.081 -15:37:58.81 AT 2026ttv 2026-07-07.42 22.5231
22:09:31.526 -19:49:15.36 AT 2026ttu 2026-07-07.39 22.923
22:25:43.683 -07:27:16.72 AT 2026ttt 2026-07-07.42 23.2007
22:23:06.784 -18:25:04.82 AT 2026tts 2026-07-07.40 22.4323
22:26:47.693 -12:06:02.25 AT 2026ttr 2026-07-07.39 22.0467
22:21:26.920 -11:44:02.24 AT 2026ttq 2026-07-07.39 22.6154
22:09:19.482 -13:54:04.50 AT 2026ttp 2026-07-07.42 22.4569
21:41:38.537 -22:07:37.94 AT 2026tto 2026-07-07.43 23.0233
22:14:46.325 -08:42:09.31 AT 2026ttn 2026-07-07.42 23.044
22:00:34.428 -18:29:27.16 AT 2026ttm 2026-07-07.42 22.0271
22:17:33.139 -16:54:49.09 AT 2026ttl 2026-07-07.42 23.3518
22:19:22.064 -20:33:27.16 AT 2026ttk 2026-07-07.40 22.5487
21:40:11.965 -23:21:51.55 AT 2026ttj 2026-07-07.40 22.0779
21:51:00.851 -19:27:38.35 AT 2026tti 2026-07-07.39 22.3735
22:16:31.668 -08:01:29.37 AT 2026tth 2026-07-07.42 22.0327
22:31:42.695 -07:14:50.87 AT 2026ttg 2026-07-07.42 22.4863
-rw-r--r-- 1 apache apache 30K Jul 14 00:21 tns_transients_list.txt
