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_021202_TTUQ2b1x1_3120339_IayKQ02p
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 13.2885 2461234.7885 11.17 23:11:50.17 +56:02:36.5
109.29296 -4.16808 galactic Cas Second-epoch detections are separated by 6.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2008809839892102016 | 23:11:49.19 +56:02:21.1 (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 23:11:50.17 +56:02:36.5: 14.97 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:11:50.17 +56:02:36.5: 14.84 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.90 +/- 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 13.2885* 23 11 50.17 +56 02 36.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2008809839892102016,2461234.7885,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2008809839892102016 20260713.2885 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.57 00:23:39.91 +53:29:32.0
118.75444 -9.15411 galactic Cas Second-epoch detections are separated by 5.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J005.9217+53.4822 | 00:23:43.87 +53:29:17.4 (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 00:23:39.91 +53:29:32.0: 14.76 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:39.91 +53:29:32.0: 15.23 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.76 +/- 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 13.2885* 00 23 39.91 +53 29 32.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J005.9217+53.4822,2461234.7885,11.57,0.05,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
ATO J005.9217+53.4822 20260713.2885 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 13.2885 2461234.7885 11.61 23:46:41.61 +54:28:42.6
113.53627 -7.20788 galactic Cas Second-epoch detections are separated by 3.2" and 5.8 pix
The object was found in VSX24" Gaia DR3 1993783609051194496
Type: VAR
# Max. Min./Amp. JD0 Period
10.550 G 10.630 G 0.017361000000 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 23:46:41.61 +54:28:42.6: 13.43 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:41.61 +54:28:42.6: 13.46 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 23 46 41.61 +54 28 42.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993783609051194496,2461234.7885,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993783609051194496 20260713.2885 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.61 00:23:06.20 +51:46:47.4
118.47652 -10.84663 galactic Cas Second-epoch detections are separated by 4.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:06.20 +51:46:47.4 (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 00:23:06.20 +51:46:47.4: 15.22 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:06.20 +51:46:47.4: 15.16 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.22 +/- 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 13.2885* 00 23 06.20 +51 46 47.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.69 23:31:49.50 +55:35:28.2
111.78753 -5.54849 galactic Cas Second-epoch detections are separated by 6.8" and 5.9 pix
The object was found in VSX18" Gaia DR3 1997656497018167168
Type: RS
# Max. Min./Amp. JD0 Period
18.500 G 18.650 G
ATTENTION: measured mag 11.69 is 6.8 mag brighter than the VSX record maximum brightness 18.50 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:31:49.50 +55:35:28.2: 13.12 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:31:49.50 +55:35:28.2: 12.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 23 31 49.50 +55 35 28.2 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 1997656497018167168,2461234.7885,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997656497018167168 20260713.2885 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.77 23:46:35.12 +54:28:36.8
113.52053 -7.20551 galactic Cas Second-epoch detections are separated by 7.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993783574691449856 | 23:46:33.09 +54:28:07.5 (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 23:46:35.12 +54:28:36.8: 14.47 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:35.12 +54:28:36.8: 14.81 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 23 46 35.12 +54 28 36.8 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 1993783574691449856,2461234.7885,11.77,0.05,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
Gaia DR3 1993783574691449856 20260713.2885 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 13.2885 2461234.7885 11.79 00:19:58.34 +51:55:30.9
118.00527 -10.64525 galactic Cas Second-epoch detections are separated by 5.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J005.0070+51.9244 | 00:19:58.34 +51:55:30.9 (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 00:19:58.34 +51:55:30.9: 13.73 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:58.34 +51:55:30.9: 13.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 00 19 58.34 +51 55 30.9 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 J005.0070+51.9244,2461234.7885,11.79,0.05,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
ATO J005.0070+51.9244 20260713.2885 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 13.2885 2461234.7885 11.79 23:36:38.52 +51:42:55.0
111.31477 -9.46142 galactic Cas Second-epoch detections are separated by 5.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J354.1561+51.7273 | 23:36:38.52 +51:42:55.0 (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 23:36:38.52 +51:42:55.0: 12.76 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:36:38.52 +51:42:55.0: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 23 36 38.52 +51 42 55.0 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 J354.1561+51.7273,2461234.7885,11.79,0.05,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
ATO J354.1561+51.7273 20260713.2885 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 13.2885 2461234.7885 11.82 23:25:20.30 +56:49:19.5
111.31894 -4.09576 galactic Cas Second-epoch detections are separated by 7.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:20.30 +56:49:19.5 (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 23:25:20.30 +56:49:19.5: 13.97 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:20.30 +56:49:19.5: 14.08 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 23 25 20.30 +56 49 19.5 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.86 23:57:30.50 +54:23:42.9
115.06025 -7.65019 galactic Cas Second-epoch detections are separated by 7.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J359.3654+54.3957 | 23:57:27.17 +54:23:10.9 (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 23:57:30.50 +54:23:42.9: 14.67 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:30.50 +54:23:42.9: 14.26 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 23 57 30.50 +54 23 42.9 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.3654+54.3957,2461234.7885,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.3654+54.3957 20260713.2885 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.83 23:21:45.74 +54:26:17.6
110.04108 -6.17363 galactic Cas Second-epoch detections are separated by 7.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.4458+54.4444 | 23:21:45.74 +54:26:17.6 (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 23:21:45.74 +54:26:17.6: 13.08 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:21:45.74 +54:26:17.6: 13.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 23 21 45.74 +54 26 17.6 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 J350.4458+54.4444,2461234.7885,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J350.4458+54.4444 20260713.2885 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 13.2885 2461234.7885 11.87 23:16:38.24 +57:25:37.4
110.41541 -3.12270 galactic Cas Second-epoch detections are separated by 6.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:16:38.24 +57:25:37.4 (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 23:16:38.24 +57:25:37.4: 13.01 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:16:38.24 +57:25:37.4: 12.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 13.2885* 23 16 38.24 +57 25 37.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 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 13.2885 2461234.7885 11.84 23:13:08.93 +56:57:55.6
109.80620 -3.38032 galactic Cas Second-epoch detections are separated by 5.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:13:08.93 +56:57:55.6 (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 23:13:08.93 +56:57:55.6: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:13:08.93 +56:57:55.6: 14.94 +/- 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 13.2885* 23 13 08.93 +56 57 55.6 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,2461234.7885,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 11.84CV 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 13.2885 2461234.7885 10.06 00:09:29.89 +51:35:56.4
116.32540 -10.73396 galactic Cas Second-epoch detections are separated by 2.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:09:29.89 +51:35:56.4 (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 00:09:29.89 +51:35:56.4: 12.43 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:09:29.89 +51:35:56.4: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 00 09 29.89 +51 35 56.4 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 10.06CV 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 13.2885 2461234.7885 12.72 00:25:08.99 +56:12:31.0
119.25883 -6.47554 galactic Cas Second-epoch detections are separated by 2.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:08.99 +56:12:31.0 (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 00:25:08.99 +56:12:31.0: 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 00:25:08.99 +56:12:31.0: 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 13.2885* 00 25 08.99 +56 12 31.0 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,2461234.7885,12.72,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.77 00:23:37.31 +55:20:26.7
118.95132 -7.31587 galactic Cas Second-epoch detections are separated by 8.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:37.31 +55:20:26.7 (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 00:23:37.31 +55:20:26.7: 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 00:23:37.31 +55:20:26.7: 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 13.2885* 00 23 37.31 +55 20 26.7 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,2461234.7885,12.77,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.79 00:31:20.89 +57:06:28.4
120.19356 -5.65701 galactic Cas Second-epoch detections are separated by 7.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:31:20.89 +57:06:28.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:20.89 +57:06:28.4: 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 00:31:20.89 +57:06:28.4: 13.40 +/- 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 13.2885* 00 31 20.89 +57 06 28.4 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,2461234.7885,12.79,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.70 00:16:33.45 +54:59:15.9
117.89806 -7.54272 galactic Cas Second-epoch detections are separated by 2.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.1344+54.9792 | 00:16:33.45 +54:59:15.9 (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 00:16:33.45 +54:59:15.9: 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 00:16:33.45 +54:59:15.9: 13.64 +/- 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 13.2885* 00 16 33.45 +54 59 15.9 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 J004.1344+54.9792,2461234.7885,12.70,0.05,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
ATO J004.1344+54.9792 20260713.2885 12.70CV 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 13.2885 2461234.7885 12.80 00:25:48.45 +51:44:26.3
118.89596 -10.93015 galactic Cas Second-epoch detections are separated by 3.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:48.45 +51:44:26.3 (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 00:25:48.45 +51:44:26.3: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:48.45 +51:44:26.3: 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 13.2885* 00 25 48.45 +51 44 26.3 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,2461234.7885,12.80,0.05,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 20260713.2885 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.76 00:19:52.20 +52:16:55.0
118.03442 -10.28936 galactic Cas Second-epoch detections are separated by 1.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:52.20 +52:16:55.0 (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 00:19:52.20 +52:16:55.0: 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 00:19:52.20 +52:16:55.0: 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 13.2885* 00 19 52.20 +52 16 55.0 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,2461234.7885,12.76,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.57 00:18:36.10 +56:44:54.8
118.41812 -5.83514 galactic Cas Second-epoch detections are separated by 7.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.6628+56.7439 | 00:18:36.10 +56:44:54.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:18:36.10 +56:44:54.8: 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 00:18:36.10 +56:44:54.8: 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 13.2885* 00 18 36.10 +56 44 54.8 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
ATO J004.6628+56.7439,2461234.7885,12.57,0.05,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
ATO J004.6628+56.7439 20260713.2885 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 13.2885 2461234.7885 12.64 00:23:50.32 +50:48:29.0
118.48354 -11.82516 galactic Cas Second-epoch detections are separated by 5.4" and 5.9 pix
The object was found in VSX25" Gaia DR3 394744676039798656
Type: S
# Max. Min./Amp. JD0 Period
17.530 G 18.140 G
ATTENTION: measured mag 12.64 is 4.9 mag brighter than the VSX record maximum brightness 17.53 - 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 00:23:50.32 +50:48:29.0: 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 00:23:50.32 +50:48:29.0: 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 13.2885* 00 23 50.32 +50 48 29.0 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 394744676039798656,2461234.7885,12.64,0.05,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
Gaia DR3 394744676039798656 20260713.2885 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 13.2885 2461234.7885 12.62 00:26:53.21 +56:55:11.3
119.56916 -5.79156 galactic Cas Second-epoch detections are separated by 4.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:53.21 +56:55:11.3 (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 00:26:53.21 +56:55:11.3: 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 00:26:53.21 +56:55:11.3: 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 13.2885* 00 26 53.21 +56 55 11.3 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,2461234.7885,12.62,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.66 00:25:28.39 +53:44:31.2
119.05108 -8.93399 galactic Cas Second-epoch detections are separated by 4.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:28.39 +53:44:31.2 (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 00:25:28.39 +53:44:31.2: 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 00:25:28.39 +53:44:31.2: 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 13.2885* 00 25 28.39 +53 44 31.2 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,2461234.7885,12.66,0.05,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
target 20260713.2885 12.66CV 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 13.2885 2461234.7885 12.68 00:25:08.57 +56:25:14.8
119.27974 -6.26439 galactic Cas Second-epoch detections are separated by 3.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:08.57 +56:25:14.8 (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 00:25:08.57 +56:25:14.8: 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 00:25:08.57 +56:25:14.8: 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 13.2885* 00 25 08.57 +56 25 14.8 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
target,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.63 00:26:39.90 +55:47:37.7
119.42943 -6.90938 galactic Cas Second-epoch detections are separated by 7.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:39.90 +55:47:37.7 (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 00:26:39.90 +55:47:37.7: 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 00:26:39.90 +55:47:37.7: 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 13.2885* 00 26 39.90 +55 47 37.7 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
target,2461234.7885,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.72 00:29:45.46 +55:26:25.4
119.83530 -7.30095 galactic Cas Second-epoch detections are separated by 7.2" and 5.7 pix
The object was found in VSX11" Gaia DR3 421240604168835712
Type: ROT
# Max. Min./Amp. JD0 Period
16.020 G 16.070 G K
ATTENTION: measured mag 12.72 is 3.3 mag brighter than the VSX record maximum brightness 16.02 - 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 00:29:45.46 +55:26:25.4: 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 00:29:45.46 +55:26:25.4: 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 13.2885* 00 29 45.46 +55 26 25.4 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 421240604168835712,2461234.7885,12.72,0.05,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
Gaia DR3 421240604168835712 20260713.2885 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 13.2885 2461234.7885 12.67 00:19:11.65 +50:41:05.8
117.72325 -11.86042 galactic Cas Second-epoch detections are separated by 2.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.7866+50.6899 | 00:19:11.65 +50:41:05.8 (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 00:19:11.65 +50:41:05.8: 13.76 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:11.65 +50:41:05.8: 13.57 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.76 +/- 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 13.2885* 00 19 11.65 +50 41 05.8 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
ATO J004.7866+50.6899,2461234.7885,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.7866+50.6899 20260713.2885 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.60 00:16:19.05 +53:07:30.1
117.60499 -9.38309 galactic Cas Second-epoch detections are separated by 1.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 419241623314205056 | 00:16:15.68 +53:07:02.8 (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 00:16:19.05 +53:07:30.1: 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 00:16:19.05 +53:07:30.1: 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 13.2885* 00 16 19.05 +53 07 30.1 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 419241623314205056,2461234.7885,12.60,0.05,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 419241623314205056 20260713.2885 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 13.2885 2461234.7885 12.55 00:28:49.63 +53:12:01.3
119.50208 -9.52074 galactic Cas Second-epoch detections are separated by 4.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:49.63 +53:12:01.3 (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 00:28:49.63 +53:12:01.3: 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 00:28:49.63 +53:12:01.3: 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 13.2885* 00 28 49.63 +53 12 01.3 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,2461234.7885,12.55,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.61 00:21:00.51 +52:22:38.5
118.22168 -10.21587 galactic Cas Second-epoch detections are separated by 5.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:00.51 +52:22:38.5 (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 00:21:00.51 +52:22:38.5: 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 00:21:00.51 +52:22:38.5: 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 13.2885* 00 21 00.51 +52 22 38.5 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
target,2461234.7885,12.61,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.59 00:21:16.93 +52:15:27.7
118.24939 -10.33967 galactic Cas Second-epoch detections are separated by 2.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J005.3013+52.2618 | 00:21:16.93 +52:15:27.7 (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 00:21:16.93 +52:15:27.7: 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 00:21:16.93 +52:15:27.7: 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 13.2885* 00 21 16.93 +52 15 27.7 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 J005.3013+52.2618,2461234.7885,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J005.3013+52.2618 20260713.2885 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.62 00:11:21.70 +52:13:52.0
116.71732 -10.15640 galactic Cas Second-epoch detections are separated by 2.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:11:21.70 +52:13:52.0 (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 00:11:21.70 +52:13:52.0: 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 00:11:21.70 +52:13:52.0: 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 13.2885* 00 11 21.70 +52 13 52.0 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,2461234.7885,12.62,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.58 00:23:42.53 +53:02:06.5
118.71054 -9.60918 galactic Cas Second-epoch detections are separated by 1.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 419087382447654400 | 00:23:40.66 +53:02:15.6 (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 00:23:42.53 +53:02:06.5: 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 00:23:42.53 +53:02:06.5: 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 13.2885* 00 23 42.53 +53 02 06.5 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 419087382447654400,2461234.7885,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 419087382447654400 20260713.2885 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 13.2885 2461234.7885 12.55 00:19:34.70 +53:55:07.7
118.19693 -8.65978 galactic Cas Second-epoch detections are separated by 2.9" and 5.9 pix
The object was found in VSX12" Gaia DR3 419698848347902976
Type: ROT
# Max. Min./Amp. JD0 Period
16.040 G 16.100 G F
ATTENTION: measured mag 12.55 is 3.5 mag brighter than the VSX record maximum brightness 16.04 - 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 00:19:34.70 +53:55:07.7: 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 00:19:34.70 +53:55:07.7: 13.47 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 19 34.70 +53 55 07.7 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
Gaia DR3 419698848347902976,2461234.7885,12.55,0.05,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
Gaia DR3 419698848347902976 20260713.2885 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 13.2885 2461234.7885 12.55 00:21:10.51 +54:55:18.0
118.55294 -7.69257 galactic Cas Second-epoch detections are separated by 2.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J005.2997+54.9189 | 00:21:10.51 +54:55:18.0 (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 00:21:10.51 +54:55:18.0: 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 00:21:10.51 +54:55:18.0: 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 13.2885* 00 21 10.51 +54 55 18.0 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 J005.2997+54.9189,2461234.7885,12.55,0.05,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 J005.2997+54.9189 20260713.2885 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 13.2885 2461234.7885 12.54 00:31:04.51 +55:56:03.4
120.06263 -6.82399 galactic Cas Second-epoch detections are separated by 7.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.7615+55.9315 | 00:31:04.51 +55:56:03.4 (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 00:31:04.51 +55:56:03.4: 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 00:31:04.51 +55:56:03.4: 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 13.2885* 00 31 04.51 +55 56 03.4 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 J007.7615+55.9315,2461234.7885,12.54,0.05,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
ATO J007.7615+55.9315 20260713.2885 12.54CV 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 13.2885 2461234.7885 12.51 00:30:00.23 +57:34:37.8
120.05011 -5.17460 galactic Cas Second-epoch detections are separated by 8.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421853994218224000 | 00:29:55.82 +57:34:19.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:00.23 +57:34:37.8: 13.60 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:00.23 +57:34:37.8: 13.37 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.60 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 30 00.23 +57 34 37.8 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 421853994218224000,2461234.7885,12.51,0.05,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 421853994218224000 20260713.2885 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 13.2885 2461234.7885 12.47 00:22:26.27 +50:18:54.7
118.20099 -12.28998 galactic Cas Second-epoch detections are separated by 6.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:26.27 +50:18:54.7 (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 00:22:26.27 +50:18:54.7: 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 00:22:26.27 +50:18:54.7: 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 13.2885* 00 22 26.27 +50 18 54.7 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,2461234.7885,12.47,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.44 00:13:44.77 +51:40:32.5
117.00022 -10.76143 galactic Cas Second-epoch detections are separated by 1.0" and 5.7 pix
The object was found in VSX22" Gaia DR3 395789280809549184
Type: ROT
# Max. Min./Amp. JD0 Period
14.920 G 14.950 G 8.543100000000 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 00:13:44.77 +51:40:32.5: 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 00:13:44.77 +51:40:32.5: 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 13.2885* 00 13 44.77 +51 40 32.5 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 395789280809549184,2461234.7885,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 395789280809549184 20260713.2885 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.32 00:20:24.11 +51:48:24.3
118.05739 -10.77101 galactic Cas Second-epoch detections are separated by 2.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 395087208274856704 | 00:20:27.19 +51:47:49.9 (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 00:20:24.11 +51:48:24.3: 13.59 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:20:24.11 +51:48:24.3: 13.16 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 20 24.11 +51 48 24.3 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 395087208274856704,2461234.7885,12.32,0.05,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 395087208274856704 20260713.2885 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 13.2885 2461234.7885 12.35 00:11:07.36 +54:58:20.1
117.11785 -7.44375 galactic Cas Second-epoch detections are separated by 8.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J001111.87+545825.6 | 00:11:11.88 +54:58:25.4 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:11:07.36 +54:58:20.1: 13.63 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:11:07.36 +54:58:20.1: 13.56 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.63 +/- 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 13.2885* 00 11 07.36 +54 58 20.1 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
ASASSN-V J001111.87+545825.6,2461234.7885,12.35,0.05,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
ASASSN-V J001111.87+545825.6 20260713.2885 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 13.2885 2461234.7885 12.37 00:23:25.61 +50:26:02.3
118.37504 -12.18977 galactic Cas Second-epoch detections are separated by 5.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:25.61 +50:26:02.3 (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 00:23:25.61 +50:26:02.3: 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 00:23:25.61 +50:26:02.3: 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 13.2885* 00 23 25.61 +50 26 02.3 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,2461234.7885,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.26 00:02:21.53 +52:42:49.5
115.43291 -9.44192 galactic Cas Second-epoch detections are separated by 3.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:02:21.53 +52:42:49.5 (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 00:02:21.53 +52:42:49.5: 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 00:02:21.53 +52:42:49.5: 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 13.2885* 00 02 21.53 +52 42 49.5 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
target,2461234.7885,12.26,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.11 00:16:40.06 +52:14:35.6
117.53556 -10.26384 galactic Cas Second-epoch detections are separated by 2.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.1610+52.2420 | 00:16:40.06 +52:14:35.6 (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 00:16:40.06 +52:14:35.6: 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 00:16:40.06 +52:14:35.6: 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 13.2885* 00 16 40.06 +52 14 35.6 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 J004.1610+52.2420,2461234.7885,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.1610+52.2420 20260713.2885 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.26 00:18:01.69 +50:32:50.2
117.51755 -11.97291 galactic Cas Second-epoch detections are separated by 4.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 394544217025761280 | 00:18:00.53 +50:32:34.2 (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 00:18:01.69 +50:32:50.2: 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 00:18:01.69 +50:32:50.2: 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 13.2885* 00 18 01.69 +50 32 50.2 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
Gaia DR3 394544217025761280,2461234.7885,12.26,0.05,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
Gaia DR3 394544217025761280 20260713.2885 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 13.2885 2461234.7885 12.28 00:24:27.31 +57:21:46.5
119.28411 -5.31760 galactic Cas Second-epoch detections are separated by 5.7" and 6.1 pix
The object was found in VSX 9" Gaia DR3 421977723637043200
Type: ROT
# Max. Min./Amp. JD0 Period
15.090 G 15.130 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 00:24:27.31 +57:21:46.5: 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 00:24:27.31 +57:21:46.5: 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 13.2885* 00 24 27.31 +57 21 46.5 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 421977723637043200,2461234.7885,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421977723637043200 20260713.2885 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.31 23:49:33.87 +55:08:18.7
114.10290 -6.66904 galactic Cas Second-epoch detections are separated by 4.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J357.3963+55.1344 | 23:49:33.87 +55:08:18.7 (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 23:49:33.87 +55:08:18.7: 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 23:49:33.87 +55:08:18.7: 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 13.2885* 23 49 33.87 +55 08 18.7 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 J357.3963+55.1344,2461234.7885,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.3963+55.1344 20260713.2885 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.36 00:27:06.63 +50:36:29.3
118.98918 -12.07728 galactic Cas Second-epoch detections are separated by 7.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:06.63 +50:36:29.3 (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 00:27:06.63 +50:36:29.3: 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 00:27:06.63 +50:36:29.3: 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 13.2885* 00 27 06.63 +50 36 29.3 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,2461234.7885,12.36,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.35 00:05:25.34 +56:43:01.1
116.61847 -5.58965 galactic Cas Second-epoch detections are separated by 6.9" 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 J001.3630+56.7153 | 00:05:25.34 +56:43:01.1 (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 00:05:25.34 +56:43:01.1: 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 00:05:25.34 +56:43:01.1: 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 13.2885* 00 05 25.34 +56 43 01.1 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
ATO J001.3630+56.7153,2461234.7885,12.35,0.05,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 J001.3630+56.7153 20260713.2885 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 13.2885 2461234.7885 12.26 00:07:15.80 +50:53:28.8
115.85207 -11.37217 galactic Cas Second-epoch detections are separated by 8.7" and 5.8 pix
The object was found in VSX21" Gaia DR3 395320098580980224
Type: ROT
# Max. Min./Amp. JD0 Period
15.270 G 15.310 G K
ATTENTION: measured mag 12.26 is 3.0 mag brighter than the VSX record maximum brightness 15.27 - 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 00:07:15.80 +50:53:28.8: 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 00:07:15.80 +50:53:28.8: 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 13.2885* 00 07 15.80 +50 53 28.8 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 395320098580980224,2461234.7885,12.26,0.05,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
Gaia DR3 395320098580980224 20260713.2885 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 13.2885 2461234.7885 12.24 00:20:47.25 +53:49:55.8
118.36514 -8.76758 galactic Cas Second-epoch detections are separated by 1.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J005.1819+53.8356 | 00:20:47.25 +53:49:55.8 (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 00:20:47.25 +53:49:55.8: 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 00:20:47.25 +53:49:55.8: 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 13.2885* 00 20 47.25 +53 49 55.8 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 J005.1819+53.8356,2461234.7885,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J005.1819+53.8356 20260713.2885 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.24 23:52:10.53 +50:21:19.9
113.35116 -11.41054 galactic Cas Second-epoch detections are separated by 6.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J358.0418+50.3527 | 23:52:10.53 +50:21:19.9 (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 23:52:10.53 +50:21:19.9: 13.51 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:52:10.53 +50:21:19.9: 13.58 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.51 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 23 52 10.53 +50 21 19.9 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 J358.0418+50.3527,2461234.7885,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.0418+50.3527 20260713.2885 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.20 00:15:11.91 +53:08:55.7
117.43994 -9.33607 galactic Cas Second-epoch detections are separated by 4.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:15:11.91 +53:08:55.7 (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 00:15:11.91 +53:08:55.7: 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 00:15:11.91 +53:08:55.7: 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 13.2885* 00 15 11.91 +53 08 55.7 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,2461234.7885,12.20,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.39 00:14:26.81 +50:19:37.6
116.90880 -12.11153 galactic Cas Second-epoch detections are separated by 5.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:14:26.81 +50:19:37.6 (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 00:14:26.81 +50:19:37.6: 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 00:14:26.81 +50:19:37.6: 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 13.2885* 00 14 26.81 +50 19 37.6 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,2461234.7885,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.97 00:15:46.28 +52:31:20.1
117.43718 -9.96857 galactic Cas Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:15:46.28 +52:31:20.1 (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 00:15:46.28 +52:31:20.1: 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 00:15:46.28 +52:31:20.1: 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 13.2885* 00 15 46.28 +52 31 20.1 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,2461234.7885,11.97,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.12 00:04:31.58 +52:54:29.4
115.79594 -9.31238 galactic Cas Second-epoch detections are separated by 7.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.1222+52.9025 | 00:04:31.58 +52:54:29.4 (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 00:04:31.58 +52:54:29.4: 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 00:04:31.58 +52:54:29.4: 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 13.2885* 00 04 31.58 +52 54 29.4 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 J001.1222+52.9025,2461234.7885,12.12,0.05,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
ATO J001.1222+52.9025 20260713.2885 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 13.2885 2461234.7885 12.19 00:17:56.73 +54:53:04.5
118.08349 -7.67156 galactic Cas Second-epoch detections are separated by 4.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 419895248613723904 | 00:17:59.55 +54:52:50.4 (Gaia DR3) | E (local) | 1.936530000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:17:56.73 +54:53:04.5: 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 00:17:56.73 +54:53:04.5: 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 13.2885* 00 17 56.73 +54 53 04.5 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
Gaia DR3 419895248613723904,2461234.7885,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419895248613723904 20260713.2885 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.02 00:06:34.62 +54:54:42.1
116.45857 -7.39522 galactic Cas Second-epoch detections are separated by 2.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:06:34.62 +54:54:42.1 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.398+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:06:34.62 +54:54:42.1: 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 00:06:34.62 +54:54:42.1: 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 13.2885* 00 06 34.62 +54 54 42.1 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,2461234.7885,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.81 23:57:47.87 +56:36:56.2
115.56626 -5.48708 galactic Cas Second-epoch detections are separated by 5.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J359.4708+56.6126 | 23:57:47.87 +56:36:56.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.499+/- (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:47.87 +56:36:56.2: 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 23:57:47.87 +56:36:56.2: 13.16 +/- 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 13.2885* 23 57 47.87 +56 36 56.2 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.4708+56.6126,2461234.7885,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.4708+56.6126 20260713.2885 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.96 00:17:42.72 +53:39:39.1
117.88683 -8.88019 galactic Cas Second-epoch detections are separated by 3.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 419363733518332928 | 00:17:45.03 +53:39:48.5 (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 00:17:42.72 +53:39:39.1: 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 00:17:42.72 +53:39:39.1: 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 13.2885* 00 17 42.72 +53 39 39.1 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 419363733518332928,2461234.7885,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419363733518332928 20260713.2885 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.90 00:21:54.66 +54:13:19.1
118.57728 -8.39993 galactic Cas Second-epoch detections are separated by 2.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 419723656079834624 | 00:21:59.08 +54:13:07.9 (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 00:21:54.66 +54:13:19.1: 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 00:21:54.66 +54:13:19.1: 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 13.2885* 00 21 54.66 +54 13 19.1 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 419723656079834624,2461234.7885,11.90,0.05,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
Gaia DR3 419723656079834624 20260713.2885 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 13.2885 2461234.7885 11.89 00:23:47.89 +51:26:19.6
118.54738 -11.19751 galactic Cas Second-epoch detections are separated by 5.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:47.89 +51:26:19.6 (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 00:23:47.89 +51:26:19.6: 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 00:23:47.89 +51:26:19.6: 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 13.2885* 00 23 47.89 +51 26 19.6 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
target,2461234.7885,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.89 00:26:32.41 +53:23:37.5
119.17551 -9.29631 galactic Cas Second-epoch detections are separated by 5.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.6517+53.3880 | 00:26:32.41 +53:23:37.5 (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 00:26:32.41 +53:23:37.5: 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 00:26:32.41 +53:23:37.5: 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 13.2885* 00 26 32.41 +53 23 37.5 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 J006.6517+53.3880,2461234.7885,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.6517+53.3880 20260713.2885 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.85 00:07:36.26 +55:01:28.7
116.62464 -7.30941 galactic Cas Second-epoch detections are separated by 5.4" and 5.9 pix
The object was found in VSX 6" Gaia DR3 420429061509672704
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.580 G 13.600 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 00:07:36.26 +55:01:28.7: 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 00:07:36.26 +55:01:28.7: 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 13.2885* 00 07 36.26 +55 01 28.7 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
Gaia DR3 420429061509672704,2461234.7885,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420429061509672704 20260713.2885 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.65 23:16:59.96 +56:24:23.4
110.09575 -4.09337 galactic Cas Second-epoch detections are separated by 7.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:16:59.96 +56:24:23.4 (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 23:16:59.96 +56:24:23.4: 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 23:16:59.96 +56:24:23.4: 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 13.2885* 23 16 59.96 +56 24 23.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.85 00:25:01.16 +55:19:54.8
119.14960 -7.34573 galactic Cas Second-epoch detections are separated by 3.8" and 5.9 pix
The object was found in VSX16" WISE J002502.5+551944
Type: EA
# Max. Min./Amp. JD0 Period
11.557 W1 Y 0.489 W1 3.154151200000
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 00:25:01.16 +55:19:54.8: 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 00:25:01.16 +55:19:54.8: 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 13.2885* 00 25 01.16 +55 19 54.8 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
WISE J002502.5+551944,2461234.7885,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J002502.5+551944 20260713.2885 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.80 00:26:03.61 +57:31:00.9
119.51559 -5.18640 galactic Cas Second-epoch detections are separated by 4.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.5159+57.5157 | 00:26:03.61 +57:31:00.9 (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 00:26:03.61 +57:31:00.9: 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 00:26:03.61 +57:31:00.9: 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 13.2885* 00 26 03.61 +57 31 00.9 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 J006.5159+57.5157,2461234.7885,11.80,0.05,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
ATO J006.5159+57.5157 20260713.2885 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
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.49 00:26:29.58 +57:34:31.3
119.57936 -5.13392 galactic Cas Second-epoch detections are separated by 7.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421889831426240768 | 00:26:29.88 +57:34:07.2 (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 00:26:29.58 +57:34:31.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:29.58 +57:34:31.3: 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 13.2885* 00 26 29.58 +57 34 31.3 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421889831426240768,2461234.7885,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421889831426240768 20260713.2885 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.54 00:08:41.39 +53:05:02.5
116.45212 -9.24905 galactic Cas Second-epoch detections are separated by 2.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:08:41.39 +53:05:02.5 (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 00:08:41.39 +53:05:02.5: 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 00:08:41.39 +53:05:02.5: 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 13.2885* 00 08 41.39 +53 05 02.5 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,2461234.7885,11.54,0.05,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 20260713.2885 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 13.2885 2461234.7885 11.55 00:21:16.64 +54:40:28.1
118.53824 -7.93978 galactic Cas Second-epoch detections are separated by 2.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:16.64 +54:40:28.1 (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 00:21:16.64 +54:40:28.1: 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 00:21:16.64 +54:40:28.1: 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 13.2885* 00 21 16.64 +54 40 28.1 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.34 00:19:51.47 +49:58:31.6
117.73900 -12.57762 galactic Cas Second-epoch detections are separated by 6.3" and 5.9 pix
The object was found in VSX20" Gaia DR3 394496422632390016
Type: ROT
# Max. Min./Amp. JD0 Period
15.320 G 15.350 G F
ATTENTION: measured mag 11.34 is 4.0 mag brighter than the VSX record maximum brightness 15.32 - 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 00:19:51.47 +49:58:31.6: 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 00:19:51.47 +49:58:31.6: 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 13.2885* 00 19 51.47 +49 58 31.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394496422632390016,2461234.7885,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 394496422632390016 20260713.2885 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.13 23:57:46.81 +52:11:11.3
114.63241 -9.81849 galactic Cas Second-epoch detections are separated by 2.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:57:46.81 +52:11:11.3 (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 23:57:46.81 +52:11:11.3: 12.42 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:46.81 +52:11:11.3: 11.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 23 57 46.81 +52 11 11.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 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 13.2885 2461234.7885 10.78 00:29:02.41 +55:22:39.7
119.72756 -7.35464 galactic Cas Second-epoch detections are separated by 1.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.2709+55.3743 | 00:29:01.39 +55:22:45.5 (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 00:29:02.41 +55:22:39.7: 13.39 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:02.41 +55:22:39.7: 12.88 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 29 02.41 +55 22 39.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J007.2709+55.3743,2461234.7885,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J007.2709+55.3743 20260713.2885 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 10.78 00:19:44.46 +51:33:12.2
117.92197 -11.00976 galactic Cas Second-epoch detections are separated by 6.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.9345+51.5528 | 00:19:44.46 +51:33:12.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.626+/-0.054 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:44.46 +51:33:12.2: 13.57 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:44.46 +51:33:12.2: 13.10 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 19 44.46 +51 33 12.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J004.9345+51.5528,2461234.7885,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.9345+51.5528 20260713.2885 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 10.53 00:17:35.04 +53:03:34.7
117.78700 -9.47359 galactic Cas Second-epoch detections are separated by 5.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.3983+53.0671 | 00:17:35.04 +53:03:34.7 (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 00:17:35.04 +53:03:34.7: 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 00:17:35.04 +53:03:34.7: 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 13.2885* 00 17 35.04 +53 03 34.7 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J004.3983+53.0671,2461234.7885,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.3983+53.0671 20260713.2885 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 9.50 00:20:43.80 +54:00:53.8
118.37885 -8.58511 galactic Cas Second-epoch detections are separated by 7.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:20:43.80 +54:00:53.8 (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 00:20:43.80 +54:00:53.8: 13.75 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:20:43.80 +54:00:53.8: 13.29 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 13.2885* 00 20 43.80 +54 00 53.8 9.5 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,2461234.7885,9.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 9.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 10.64 23:57:09.66 +50:28:26.1
114.16803 -11.47195 galactic Cas Second-epoch detections are separated by 8.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:57:09.66 +50:28:26.1 (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 23:57:09.66 +50:28:26.1: 12.52 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:09.66 +50:28:26.1: 12.10 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 23 57 09.66 +50 28 26.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 10.98 00:13:39.50 +56:53:46.2
117.76525 -5.59611 galactic Cas Second-epoch detections are separated by 5.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J003.4030+56.9099 | 00:13:37.40 +56:53:50.8 (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 00:13:39.50 +56:53:46.2: 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 00:13:39.50 +56:53:46.2: 13.28 +/- 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 13.2885* 00 13 39.50 +56 53 46.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.4030+56.9099,2461234.7885,10.98,0.05,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
ATO J003.4030+56.9099 20260713.2885 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 13.2885 2461234.7885 10.82 00:25:19.81 +55:26:51.3
119.20583 -7.23517 galactic Cas Second-epoch detections are separated by 6.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421200575075765504 | 00:25:23.67 +55:26:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:19.81 +55:26:51.3: 12.77 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:19.81 +55:26:51.3: 12.27 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 13.2885* 00 25 19.81 +55 26 51.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421200575075765504,2461234.7885,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421200575075765504 20260713.2885 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.31 00:19:32.75 +57:40:55.6
118.66346 -4.92508 galactic Cas Second-epoch detections are separated by 8.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 422040911198672384 | 00:19:36.72 +57:40:36.0 (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 00:19:32.75 +57:40:55.6: 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 00:19:32.75 +57:40:55.6: 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 13.2885* 00 19 32.75 +57 40 55.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 422040911198672384,2461234.7885,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 422040911198672384 20260713.2885 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.44 00:31:44.06 +56:11:45.7
120.17560 -6.57024 galactic Cas Second-epoch detections are separated by 4.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 418658263673436672 | 00:31:40.13 +56:11:54.6 (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 00:31:44.06 +56:11:45.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:44.06 +56:11:45.7: 13.30 +/- 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 13.2885* 00 31 44.06 +56 11 45.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 418658263673436672,2461234.7885,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 418658263673436672 20260713.2885 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.50 00:17:26.62 +49:47:25.8
117.31918 -12.71042 galactic Cas Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:17:26.62 +49:47:25.8 (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 00:17:26.62 +49:47:25.8: 13.03 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:17:26.62 +49:47:25.8: 12.97 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 17 26.62 +49 47 25.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.48 00:07:57.56 +52:30:05.1
116.24205 -9.80467 galactic Cas Second-epoch detections are separated by 3.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:07:57.56 +52:30:05.1 (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 00:07:57.56 +52:30:05.1: 13.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:57.56 +52:30:05.1: 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 13.2885* 00 07 57.56 +52 30 05.1 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,2461234.7885,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 11.74 23:52:40.10 +50:22:49.0
113.43500 -11.40464 galactic Cas Second-epoch detections are separated by 7.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1940909812857259648 | 23:52:35.86 +50:22:52.9 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:52:40.10 +50:22:49.0: 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 23:52:40.10 +50:22:49.0: 12.82 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 23 52 40.10 +50 22 49.0 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 1940909812857259648,2461234.7885,11.74,0.05,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 1940909812857259648 20260713.2885 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 13.2885 2461234.7885 11.93 00:26:25.79 +51:06:49.6
118.93043 -11.56357 galactic Cas Second-epoch detections are separated by 7.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:25.79 +51:06:49.6 (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 00:26:25.79 +51:06:49.6: 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 00:26:25.79 +51:06:49.6: 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 13.2885* 00 26 25.79 +51 06 49.6 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
target,2461234.7885,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260713.2885 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 13.2885 2461234.7885 11.81 23:33:26.19 +50:19:13.1
110.40667 -10.64485 galactic And Second-epoch detections are separated by 2.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:33:26.19 +50:19:13.1 (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 23:33:26.19 +50:19:13.1: 13.08 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:33:26.19 +50:19:13.1: 12.86 +/- 0.20 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 23 33 26.19 +50 19 13.1 11.8 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
target,2461234.7885,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.04 00:27:57.22 +51:38:49.2
119.22391 -11.05559 galactic Cas Second-epoch detections are separated by 7.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:57.22 +51:38:49.2 (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 00:27:57.22 +51:38:49.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:57.22 +51:38:49.2: 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 13.2885* 00 27 57.22 +51 38 49.2 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,2461234.7885,12.04,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.03 00:09:05.15 +53:32:52.1
116.58929 -8.80157 galactic Cas Second-epoch detections are separated by 8.2" and 5.8 pix
The object was found in VSX22" ZTF J000902.77+533244.4
Type: EA
# Max. Min./Amp. JD0 Period
18.636 r Y 0.523 r 2458363.78280 0.777391600000
ATTENTION: measured mag 12.03 is 6.1 mag brighter than the VSX record maximum brightness 18.11 - 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 00:09:05.15 +53:32:52.1: 13.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:09:05.15 +53:32:52.1: 13.69 +/- 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 13.2885* 00 09 05.15 +53 32 52.1 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
ZTF J000902.77+533244.4,2461234.7885,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J000902.77+533244.4 20260713.2885 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.16 00:24:17.17 +51:18:55.2
118.61094 -11.32847 galactic Cas Second-epoch detections are separated by 4.5" and 5.8 pix
The object was found in VSX13" Gaia DR3 394827826603556864
Type: RR
# Max. Min./Amp. JD0 Period
19.990 G 20.570 G
ATTENTION: measured mag 12.16 is 7.8 mag brighter than the VSX record maximum brightness 19.99 - 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 00:24:17.17 +51:18:55.2: 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 00:24:17.17 +51:18:55.2: 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 13.2885* 00 24 17.17 +51 18 55.2 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
Gaia DR3 394827826603556864,2461234.7885,12.16,0.05,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
Gaia DR3 394827826603556864 20260713.2885 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 13.2885 2461234.7885 12.10 00:30:06.96 +55:40:15.5
119.90572 -7.07544 galactic Cas Second-epoch detections are separated by 3.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421264621626812288 | 00:30:09.72 +55:39:51.5 (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 00:30:06.96 +55:40:15.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:06.96 +55:40:15.5: 13.33 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 30 06.96 +55 40 15.5 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 421264621626812288,2461234.7885,12.10,0.05,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
Gaia DR3 421264621626812288 20260713.2885 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 13.2885 2461234.7885 12.06 00:18:22.11 +56:40:04.9
118.37585 -5.91090 galactic Cas Second-epoch detections are separated by 6.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421594097150660352 | 00:18:20.70 +56:40:25.0 (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 00:18:22.11 +56:40:04.9: 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 00:18:22.11 +56:40:04.9: 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 13.2885* 00 18 22.11 +56 40 04.9 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 421594097150660352,2461234.7885,12.06,0.05,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
Gaia DR3 421594097150660352 20260713.2885 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 13.2885 2461234.7885 12.13 00:30:59.57 +57:25:04.4
120.17004 -5.34418 galactic Cas Second-epoch detections are separated by 5.6" and 5.8 pix
The object was found in VSX 5" Gaia DR3 421839975445105536
Type: E
# Max. Min./Amp. JD0 Period
13.480 G 13.690 G 2.085110000000 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 00:30:59.57 +57:25:04.4: 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 00:30:59.57 +57:25:04.4: 13.40 +/- 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 13.2885* 00 30 59.57 +57 25 04.4 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 421839975445105536,2461234.7885,12.13,0.05,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 421839975445105536 20260713.2885 12.13CV 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 13.2885 2461234.7885 12.27 00:27:16.60 +50:21:07.3
118.99091 -12.33475 galactic Cas Second-epoch detections are separated by 7.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.8088+50.3432 | 00:27:16.60 +50:21:07.3 (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 00:27:16.60 +50:21:07.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:16.60 +50:21:07.3: 13.40 +/- 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 13.2885* 00 27 16.60 +50 21 07.3 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 J006.8088+50.3432,2461234.7885,12.27,0.05,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
ATO J006.8088+50.3432 20260713.2885 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 13.2885 2461234.7885 12.34 00:26:50.34 +50:01:56.9
118.88782 -12.64602 galactic Cas Second-epoch detections are separated by 7.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:50.34 +50:01:56.9 (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 00:26:50.34 +50:01:56.9: 13.40 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:50.34 +50:01:56.9: 13.23 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.40 +/- 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 13.2885* 00 26 50.34 +50 01 56.9 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
target,2461234.7885,12.34,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.14 00:23:52.33 +53:12:05.9
118.75358 -9.44633 galactic Cas Second-epoch detections are separated by 2.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:52.33 +53:12:05.9 (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 00:23:52.33 +53:12:05.9: 13.56 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:52.33 +53:12:05.9: 13.27 +/- 0.29 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 23 52.33 +53 12 05.9 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
target,2461234.7885,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.38 00:24:32.66 +50:12:45.2
118.53186 -12.42929 galactic Cas Second-epoch detections are separated by 6.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:32.66 +50:12:45.2 (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 00:24:32.66 +50:12:45.2: 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 00:24:32.66 +50:12:45.2: 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 13.2885* 00 24 32.66 +50 12 45.2 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
target,2461234.7885,12.38,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.21 00:05:35.28 +53:09:22.8
116.00052 -9.09725 galactic Cas Second-epoch detections are separated by 8.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:05:35.28 +53:09:22.8 (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 00:05:35.28 +53:09:22.8: 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 00:05:35.28 +53:09:22.8: 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 13.2885* 00 05 35.28 +53 09 22.8 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,2461234.7885,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.15 00:28:36.83 +57:13:19.5
119.83203 -5.51223 galactic Cas Second-epoch detections are separated by 5.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421822520696970496 | 00:28:33.81 +57:13:25.5 (Gaia DR3) | ROT (local) | 1.040080000000 (local) | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:36.83 +57:13:19.5: 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 00:28:36.83 +57:13:19.5: 13.22 +/- 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 13.2885* 00 28 36.83 +57 13 19.5 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
Gaia DR3 421822520696970496,2461234.7885,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421822520696970496 20260713.2885 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.34 00:25:21.82 +52:37:58.0
118.91957 -10.03572 galactic Cas Second-epoch detections are separated by 2.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:21.82 +52:37:58.0 (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 00:25:21.82 +52:37:58.0: 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 00:25:21.82 +52:37:58.0: 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 13.2885* 00 25 21.82 +52 37 58.0 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
target,2461234.7885,12.34,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.33 00:31:11.03 +55:35:42.6
120.05087 -7.16324 galactic Cas Second-epoch detections are separated by 3.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:31:11.03 +55:35:42.6 (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 00:31:11.03 +55:35:42.6: 13.60 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:11.03 +55:35:42.6: 13.13 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 31 11.03 +55 35 42.6 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
target,2461234.7885,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.46 00:30:02.61 +57:31:36.2
120.05121 -5.22531 galactic Cas Second-epoch detections are separated by 8.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.4908+57.5416 | 00:30:02.18 +57:32:19.3 (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 00:30:02.61 +57:31:36.2: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:02.61 +57:31:36.2: 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 13.2885* 00 30 02.61 +57 31 36.2 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 J007.4908+57.5416,2461234.7885,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J007.4908+57.5416 20260713.2885 12.46CV 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 13.2885 2461234.7885 12.43 00:25:27.09 +50:00:26.5
118.65797 -12.64862 galactic Cas Second-epoch detections are separated by 7.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 394635858746747392 | 00:25:26.24 +50:00:10.7 (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 00:25:27.09 +50:00:26.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:27.09 +50:00:26.5: 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 13.2885* 00 25 27.09 +50 00 26.5 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 394635858746747392,2461234.7885,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 394635858746747392 20260713.2885 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.56 00:28:32.21 +51:40:59.2
119.31903 -11.02792 galactic Cas Second-epoch detections are separated by 5.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.1490+51.6864 | 00:28:32.21 +51:40:59.2 (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 00:28:32.21 +51:40:59.2: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:32.21 +51:40:59.2: 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 13.2885* 00 28 32.21 +51 40 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
ATO J007.1490+51.6864,2461234.7885,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J007.1490+51.6864 20260713.2885 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.46 00:30:26.43 +55:57:29.1
119.97538 -6.79308 galactic Cas Second-epoch detections are separated by 5.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.6174+55.9537 | 00:30:26.43 +55:57:29.1 (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 00:30:26.43 +55:57:29.1: 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 00:30:26.43 +55:57:29.1: 13.40 +/- 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 13.2885* 00 30 26.43 +55 57 29.1 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
ATO J007.6174+55.9537,2461234.7885,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J007.6174+55.9537 20260713.2885 12.46CV 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 13.2885 2461234.7885 12.51 00:28:43.64 +53:35:06.8
119.52178 -9.13609 galactic Cas Second-epoch detections are separated by 1.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:43.64 +53:35:06.8 (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 00:28:43.64 +53:35:06.8: 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 00:28:43.64 +53:35:06.8: 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 13.2885* 00 28 43.64 +53 35 06.8 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,2461234.7885,12.51,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.42 00:31:11.54 +56:01:45.2
120.08667 -6.73064 galactic Cas Second-epoch detections are separated by 7.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421652130754837120 | 00:31:11.21 +56:01:00.3 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:11.54 +56:01:45.2: 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 00:31:11.54 +56:01:45.2: 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 13.2885* 00 31 11.54 +56 01 45.2 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 421652130754837120,2461234.7885,12.42,0.05,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
Gaia DR3 421652130754837120 20260713.2885 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 13.2885 2461234.7885 12.65 00:28:15.30 +52:44:18.1
119.37281 -9.97311 galactic Cas Second-epoch detections are separated by 3.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:15.30 +52:44:18.1 (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 00:28:15.30 +52:44:18.1: 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 00:28:15.30 +52:44:18.1: 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 13.2885* 00 28 15.30 +52 44 18.1 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,2461234.7885,12.65,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.45 00:30:30.72 +55:12:22.2
119.92344 -7.54330 galactic Cas Second-epoch detections are separated by 3.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:30:30.72 +55:12:22.2 (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 00:30:30.72 +55:12:22.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:30.72 +55:12:22.2: 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 13.2885* 00 30 30.72 +55 12 22.2 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
target,2461234.7885,12.45,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.45 00:17:29.39 +52:44:47.7
117.73048 -9.78197 galactic Cas Second-epoch detections are separated by 1.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:17:29.39 +52:44:47.7 (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 00:17:29.39 +52:44:47.7: 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 00:17:29.39 +52:44:47.7: 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 13.2885* 00 17 29.39 +52 44 47.7 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,2461234.7885,12.45,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.41 00:19:26.56 +54:51:21.8
118.29536 -7.72740 galactic Cas Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:26.56 +54:51:21.8 (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 00:19:26.56 +54:51:21.8: 13.52 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:26.56 +54:51:21.8: 13.55 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.52 +/- 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 13.2885* 00 19 26.56 +54 51 21.8 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,2461234.7885,12.41,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.43 00:31:08.08 +57:01:57.2
120.15853 -5.72982 galactic Cas Second-epoch detections are separated by 5.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:31:08.08 +57:01:57.2 (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 00:31:08.08 +57:01:57.2: 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 00:31:08.08 +57:01:57.2: 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 13.2885* 00 31 08.08 +57 01 57.2 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
target,2461234.7885,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.70 00:24:55.10 +50:43:56.9
118.64869 -11.91859 galactic Cas Second-epoch detections are separated by 1.1" and 5.3 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 | 00:24:55.10 +50:43:56.9 (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 00:24:55.10 +50:43:56.9: 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 00:24:55.10 +50:43:56.9: 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 13.2885* 00 24 55.10 +50 43 56.9 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,2461234.7885,12.70,0.05,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 20260713.2885 12.70CV 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 13.2885 2461234.7885 12.54 00:31:58.07 +57:30:55.6
120.30890 -5.25711 galactic Cas Second-epoch detections are separated by 7.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.9945+57.5159 | 00:31:56.54 +57:31:38.2 (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 00:31:58.07 +57:30:55.6: 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 00:31:58.07 +57:30:55.6: 13.40 +/- 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 13.2885* 00 31 58.07 +57 30 55.6 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 J007.9945+57.5159,2461234.7885,12.54,0.05,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
ATO J007.9945+57.5159 20260713.2885 12.54CV 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 13.2885 2461234.7885 12.45 00:16:18.03 +55:02:57.1
117.86972 -7.47682 galactic Cas Second-epoch detections are separated by 2.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:16:18.03 +55:02:57.1 (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 00:16:18.03 +55:02:57.1: 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 00:16:18.03 +55:02:57.1: 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 13.2885* 00 16 18.03 +55 02 57.1 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,2461234.7885,12.45,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.67 00:24:33.64 +50:28:22.8
118.56293 -12.17061 galactic Cas Second-epoch detections are separated by 4.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:33.64 +50:28:22.8 (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 00:24:33.64 +50:28:22.8: 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 00:24:33.64 +50:28:22.8: 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 13.2885* 00 24 33.64 +50 28 22.8 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
target,2461234.7885,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.56 00:24:19.22 +49:57:03.6
118.46653 -12.68549 galactic Cas Second-epoch detections are separated by 8.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:19.22 +49:57:03.6 (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 00:24:19.22 +49:57:03.6: 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 00:24:19.22 +49:57:03.6: 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 13.2885* 00 24 19.22 +49 57 03.6 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,2461234.7885,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.31 00:24:27.91 +57:11:49.9
119.26798 -5.48255 galactic Cas Second-epoch detections are separated by 4.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.0891+57.1981 | 00:24:24.73 +57:11:52.7 (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 00:24:27.91 +57:11:49.9: 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 00:24:27.91 +57:11:49.9: 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 13.2885* 00 24 27.91 +57 11 49.9 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 J006.0891+57.1981,2461234.7885,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.0891+57.1981 20260713.2885 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.64 00:32:02.90 +57:43:25.8
120.33553 -5.05013 galactic Cas Second-epoch detections are separated by 8.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.9868+57.7272 | 00:31:59.43 +57:43:23.8 (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 00:32:02.90 +57:43:25.8: 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 00:32:02.90 +57:43:25.8: 13.36 +/- 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 13.2885* 00 32 02.90 +57 43 25.8 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
ATO J007.9868+57.7272,2461234.7885,12.64,0.05,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 J007.9868+57.7272 20260713.2885 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 13.2885 2461234.7885 12.48 23:32:13.83 +53:34:05.7
111.22441 -7.49339 galactic Cas Second-epoch detections are separated by 6.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.0553+53.5633 | 23:32:13.83 +53:34:05.7 (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 23:32:13.83 +53:34:05.7: 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 23:32:13.83 +53:34:05.7: 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 13.2885* 23 32 13.83 +53 34 05.7 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 J353.0553+53.5633,2461234.7885,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.0553+53.5633 20260713.2885 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.45 00:10:15.52 +53:28:38.1
116.75172 -8.89964 galactic Cas Second-epoch detections are separated by 2.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:10:15.52 +53:28:38.1 (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 00:10:15.52 +53:28:38.1: 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 00:10:15.52 +53:28:38.1: 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 13.2885* 00 10 15.52 +53 28 38.1 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,2461234.7885,12.45,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.70 00:16:09.79 +50:03:00.1
117.14651 -12.42505 galactic Cas Second-epoch detections are separated by 7.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:16:09.79 +50:03:00.1 (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 00:16:09.79 +50:03:00.1: 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 00:16:09.79 +50:03:00.1: 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 13.2885* 00 16 09.79 +50 03 00.1 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,2461234.7885,12.70,0.05,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 20260713.2885 12.70CV 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 13.2885 2461234.7885 12.44 00:25:19.19 +57:25:08.3
119.40629 -5.27388 galactic Cas Second-epoch detections are separated by 8.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.3264+57.4197 | 00:25:19.19 +57:25:08.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.838+/-0.031 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:19.19 +57:25:08.3: 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 00:25:19.19 +57:25:08.3: 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 13.2885* 00 25 19.19 +57 25 08.3 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 J006.3264+57.4197,2461234.7885,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.3264+57.4197 20260713.2885 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.55 00:13:35.35 +52:46:38.3
117.14214 -9.66844 galactic Cas Second-epoch detections are separated by 2.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:13:35.35 +52:46:38.3 (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 00:13:35.35 +52:46:38.3: 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 00:13:35.35 +52:46:38.3: 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 13.2885* 00 13 35.35 +52 46 38.3 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,2461234.7885,12.55,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.68 00:25:30.01 +49:43:57.0
118.63689 -12.92282 galactic Cas Second-epoch detections are separated by 7.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:30.01 +49:43:57.0 (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 00:25:30.01 +49:43:57.0: 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 00:25:30.01 +49:43:57.0: 13.36 +/- 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 13.2885* 00 25 30.01 +49 43 57.0 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,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.64 00:27:39.18 +50:22:51.4
119.05487 -12.31167 galactic Cas Second-epoch detections are separated by 5.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391671163083380992 | 00:27:36.91 +50:23:24.5 (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 00:27:39.18 +50:22:51.4: 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 00:27:39.18 +50:22:51.4: 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 13.2885* 00 27 39.18 +50 22 51.4 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 391671163083380992,2461234.7885,12.64,0.05,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
Gaia DR3 391671163083380992 20260713.2885 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 13.2885 2461234.7885 12.53 00:22:01.91 +51:22:31.0
118.26106 -11.22959 galactic Cas Second-epoch detections are separated by 2.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:01.91 +51:22:31.0 (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 00:22:01.91 +51:22:31.0: 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 00:22:01.91 +51:22:31.0: 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 13.2885* 00 22 01.91 +51 22 31.0 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,2461234.7885,12.53,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.55 00:28:04.73 +57:36:04.4
119.79421 -5.12815 galactic Cas Second-epoch detections are separated by 7.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:04.73 +57:36:04.4 (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 00:28:04.73 +57:36:04.4: 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 00:28:04.73 +57:36:04.4: 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 13.2885* 00 28 04.73 +57 36 04.4 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,2461234.7885,12.55,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.67 00:22:40.91 +50:29:36.0
118.26136 -12.11746 galactic Cas Second-epoch detections are separated by 5.1" and 5.9 pix
The object was found in VSX24" Gaia DR3 394712446603310848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
17.130 G 17.220 G G
ATTENTION: measured mag 12.67 is 4.5 mag brighter than the VSX record maximum brightness 17.13 - 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 00:22:40.91 +50:29:36.0: 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 00:22:40.91 +50:29:36.0: 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 13.2885* 00 22 40.91 +50 29 36.0 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
Gaia DR3 394712446603310848,2461234.7885,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 394712446603310848 20260713.2885 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.70 00:26:30.66 +57:24:44.4
119.56589 -5.29641 galactic Cas Second-epoch detections are separated by 5.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:30.66 +57:24:44.4 (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 00:26:30.66 +57:24:44.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:30.66 +57:24:44.4: 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 13.2885* 00 26 30.66 +57 24 44.4 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,2461234.7885,12.70,0.05,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 20260713.2885 12.70CV 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 13.2885 2461234.7885 12.60 00:15:38.78 +53:48:04.1
117.59989 -8.69966 galactic Cas Second-epoch detections are separated by 3.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 419357518709533824 | 00:15:42.50 +53:47:45.8 (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 00:15:38.78 +53:48:04.1: 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 00:15:38.78 +53:48:04.1: 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 13.2885* 00 15 38.78 +53 48 04.1 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 419357518709533824,2461234.7885,12.60,0.05,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 419357518709533824 20260713.2885 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 13.2885 2461234.7885 12.56 00:26:09.86 +50:22:56.2
118.81326 -12.28725 galactic Cas Second-epoch detections are separated by 5.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:09.86 +50:22:56.2 (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 00:26:09.86 +50:22:56.2: 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 00:26:09.86 +50:22:56.2: 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 13.2885* 00 26 09.86 +50 22 56.2 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,2461234.7885,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.62 00:25:53.58 +53:52:55.2
119.12779 -8.80096 galactic Cas Second-epoch detections are separated by 4.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:53.58 +53:52:55.2 (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 00:25:53.58 +53:52:55.2: 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 00:25:53.58 +53:52:55.2: 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 13.2885* 00 25 53.58 +53 52 55.2 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,2461234.7885,12.62,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.54 00:24:54.84 +54:39:08.3
119.06346 -8.02010 galactic Cas Second-epoch detections are separated by 3.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:54.84 +54:39:08.3 (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 00:24:54.84 +54:39:08.3: 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 00:24:54.84 +54:39:08.3: 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 13.2885* 00 24 54.84 +54 39 08.3 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,2461234.7885,12.54,0.05,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 20260713.2885 12.54CV 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 13.2885 2461234.7885 12.68 00:25:29.74 +55:20:20.4
119.21827 -7.34558 galactic Cas Second-epoch detections are separated by 6.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:29.74 +55:20:20.4 (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 00:25:29.74 +55:20:20.4: 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 00:25:29.74 +55:20:20.4: 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 13.2885* 00 25 29.74 +55 20 20.4 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,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.58 00:24:26.76 +55:37:43.0
119.09937 -7.04215 galactic Cas Second-epoch detections are separated by 1.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.1281+55.6288 | 00:24:26.76 +55:37:43.0 (user input) | NSINE (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 00:24:26.76 +55:37:43.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:24:26.76 +55:37:43.0: 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 13.2885* 00 24 26.76 +55 37 43.0 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 J006.1281+55.6288,2461234.7885,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J006.1281+55.6288 20260713.2885 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 13.2885 2461234.7885 12.68 00:17:58.75 +53:30:39.8
117.90666 -9.03391 galactic Cas Second-epoch detections are separated by 1.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:17:58.75 +53:30:39.8 (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 00:17:58.75 +53:30:39.8: 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 00:17:58.75 +53:30:39.8: 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 13.2885* 00 17 58.75 +53 30 39.8 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
target,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.58 00:21:18.69 +51:09:17.7
118.12051 -11.43517 galactic Cas Second-epoch detections are separated by 3.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:18.69 +51:09:17.7 (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 00:21:18.69 +51:09:17.7: 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 00:21:18.69 +51:09:17.7: 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 13.2885* 00 21 18.69 +51 09 17.7 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
target,2461234.7885,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260713.2885 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 13.2885 2461234.7885 12.69 00:28:36.32 +52:45:09.1
119.42772 -9.96380 galactic Cas Second-epoch detections are separated by 7.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:36.32 +52:45:09.1 (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 00:28:36.32 +52:45:09.1: 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 00:28:36.32 +52:45:09.1: 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 13.2885* 00 28 36.32 +52 45 09.1 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,2461234.7885,12.69,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.62 00:18:39.72 +50:29:11.2
117.61153 -12.04641 galactic Cas Second-epoch detections are separated by 1.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:39.72 +50:29:11.2 (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 00:18:39.72 +50:29:11.2: 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 00:18:39.72 +50:29:11.2: 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 13.2885* 00 18 39.72 +50 29 11.2 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,2461234.7885,12.62,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.76 00:26:48.99 +50:20:31.3
118.91512 -12.33759 galactic Cas Second-epoch detections are separated by 5.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:48.99 +50:20:31.3 (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 00:26:48.99 +50:20:31.3: 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 00:26:48.99 +50:20:31.3: 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 13.2885* 00 26 48.99 +50 20 31.3 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,2461234.7885,12.76,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.49 00:18:09.60 +50:01:26.6
117.46822 -12.49433 galactic Cas Second-epoch detections are separated by 2.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:09.60 +50:01:26.6 (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 00:18:09.60 +50:01:26.6: 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 00:18:09.60 +50:01:26.6: 13.40 +/- 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 13.2885* 00 18 09.60 +50 01 26.6 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,2461234.7885,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.58 00:10:39.55 +50:02:31.4
116.25099 -12.29997 galactic Cas Second-epoch detections are separated by 7.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:10:39.55 +50:02:31.4 (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 00:10:39.55 +50:02:31.4: 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 00:10:39.55 +50:02:31.4: 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 13.2885* 00 10 39.55 +50 02 31.4 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,2461234.7885,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260713.2885 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 13.2885 2461234.7885 12.62 00:19:08.44 +52:18:48.1
117.92600 -10.24419 galactic Cas Second-epoch detections are separated by 2.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:08.44 +52:18:48.1 (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 00:19:08.44 +52:18:48.1: 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 00:19:08.44 +52:18:48.1: 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 13.2885* 00 19 08.44 +52 18 48.1 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,2461234.7885,12.62,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.60 00:18:11.77 +53:11:42.1
117.89733 -9.35146 galactic Cas Second-epoch detections are separated by 1.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:11.77 +53:11:42.1 (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 00:18:11.77 +53:11:42.1: 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 00:18:11.77 +53:11:42.1: 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 13.2885* 00 18 11.77 +53 11 42.1 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,2461234.7885,12.60,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.69 00:26:38.20 +51:44:56.0
119.02687 -10.93471 galactic Cas Second-epoch detections are separated by 2.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:38.20 +51:44:56.0 (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 00:26:38.20 +51:44:56.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:38.20 +51:44:56.0: 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 13.2885* 00 26 38.20 +51 44 56.0 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,2461234.7885,12.69,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.56 00:23:32.61 +55:48:00.5
118.99057 -6.85800 galactic Cas Second-epoch detections are separated by 4.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:32.61 +55:48:00.5 (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 00:23:32.61 +55:48:00.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:32.61 +55:48:00.5: 13.40 +/- 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 13.2885* 00 23 32.61 +55 48 00.5 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
target,2461234.7885,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.63 00:27:57.97 +51:44:12.5
119.23436 -10.96635 galactic Cas Second-epoch detections are separated by 5.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.9891+51.7361 | 00:27:57.97 +51:44:12.5 (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 00:27:57.97 +51:44:12.5: 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 00:27:57.97 +51:44:12.5: 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 13.2885* 00 27 57.97 +51 44 12.5 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
ATO J006.9891+51.7361,2461234.7885,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.9891+51.7361 20260713.2885 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.67 00:23:54.91 +50:22:50.0
118.44816 -12.25143 galactic Cas Second-epoch detections are separated by 4.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:23:54.91 +50:22:50.0 (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 00:23:54.91 +50:22:50.0: 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 00:23:54.91 +50:22:50.0: 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 13.2885* 00 23 54.91 +50 22 50.0 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,2461234.7885,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.62 00:27:16.82 +49:54:40.3
118.94818 -12.77360 galactic Cas Second-epoch detections are separated by 7.0" and 5.8 pix
The object was found in VSX20" Gaia DR3 391633779687377536
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.790 G 13.840 G 0.023889600000 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 00:27:16.82 +49:54:40.3: 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 00:27:16.82 +49:54:40.3: 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 13.2885* 00 27 16.82 +49 54 40.3 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
Gaia DR3 391633779687377536,2461234.7885,12.62,0.05,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
Gaia DR3 391633779687377536 20260713.2885 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 13.2885 2461234.7885 12.70 00:25:25.68 +49:53:23.2
118.64167 -12.76518 galactic Cas Second-epoch detections are separated by 7.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 394633625365572736 | 00:25:25.03 +49:53:42.1 (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 00:25:25.68 +49:53:23.2: 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 00:25:25.68 +49:53:23.2: 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 13.2885* 00 25 25.68 +49 53 23.2 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 394633625365572736,2461234.7885,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 394633625365572736 20260713.2885 12.70CV 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 13.2885 2461234.7885 12.62 00:24:26.36 +53:32:29.6
118.87569 -9.11743 galactic Cas Second-epoch detections are separated by 2.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 419481724859223680 | 00:24:28.68 +53:32:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:24:26.36 +53:32:29.6: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:24:26.36 +53:32:29.6: 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 13.2885* 00 24 26.36 +53 32 29.6 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 419481724859223680,2461234.7885,12.62,0.05,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
Gaia DR3 419481724859223680 20260713.2885 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 13.2885 2461234.7885 12.73 00:25:48.36 +53:57:27.4
119.12257 -8.72445 galactic Cas Second-epoch detections are separated by 3.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:48.36 +53:57:27.4 (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 00:25:48.36 +53:57:27.4: 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 00:25:48.36 +53:57:27.4: 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 13.2885* 00 25 48.36 +53 57 27.4 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,2461234.7885,12.73,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.71 00:22:25.25 +51:23:55.3
118.32527 -11.21333 galactic Cas Second-epoch detections are separated by 4.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:25.25 +51:23:55.3 (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 00:22:25.25 +51:23:55.3: 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 00:22:25.25 +51:23:55.3: 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 13.2885* 00 22 25.25 +51 23 55.3 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,2461234.7885,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.54 00:20:50.70 +50:44:15.7
117.99491 -11.84056 galactic Cas Second-epoch detections are separated by 3.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:20:50.70 +50:44:15.7 (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 00:20:50.70 +50:44:15.7: 13.50 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:20:50.70 +50:44:15.7: 13.46 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.50 +/- 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 13.2885* 00 20 50.70 +50 44 15.7 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,2461234.7885,12.54,0.05,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 20260713.2885 12.54CV 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 13.2885 2461234.7885 12.68 00:25:34.05 +51:58:55.4
118.88340 -10.68622 galactic Cas Second-epoch detections are separated by 4.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:34.05 +51:58:55.4 (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 00:25:34.05 +51:58:55.4: 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 00:25:34.05 +51:58:55.4: 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 13.2885* 00 25 34.05 +51 58 55.4 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,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.71 00:19:43.91 +51:43:50.6
117.94310 -10.83364 galactic Cas Second-epoch detections are separated by 2.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:43.91 +51:43:50.6 (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 00:19:43.91 +51:43:50.6: 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 00:19:43.91 +51:43:50.6: 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 13.2885* 00 19 43.91 +51 43 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
target,2461234.7885,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.71 00:24:23.63 +50:19:40.3
118.52000 -12.31207 galactic Cas Second-epoch detections are separated by 5.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.0919+50.3367 | 00:24:23.63 +50:19:40.3 (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 00:24:23.63 +50:19:40.3: 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 00:24:23.63 +50:19:40.3: 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 13.2885* 00 24 23.63 +50 19 40.3 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
ATO J006.0919+50.3367,2461234.7885,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.0919+50.3367 20260713.2885 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.66 00:28:27.49 +52:13:56.6
119.35736 -10.47980 galactic Cas Second-epoch detections are separated by 5.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:27.49 +52:13:56.6 (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 00:28:27.49 +52:13:56.6: 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 00:28:27.49 +52:13:56.6: 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 13.2885* 00 28 27.49 +52 13 56.6 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,2461234.7885,12.66,0.05,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
target 20260713.2885 12.66CV 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 13.2885 2461234.7885 12.67 00:25:02.99 +53:23:18.1
118.95097 -9.27930 galactic Cas Second-epoch detections are separated by 4.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:02.99 +53:23:18.1 (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 00:25:02.99 +53:23:18.1: 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 00:25:02.99 +53:23:18.1: 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 13.2885* 00 25 02.99 +53 23 18.1 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,2461234.7885,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.68 00:27:19.19 +57:11:04.1
119.65327 -5.53366 galactic Cas Second-epoch detections are separated by 3.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:19.19 +57:11:04.1 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:19.19 +57:11:04.1: 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 00:27:19.19 +57:11:04.1: 13.40 +/- 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 13.2885* 00 27 19.19 +57 11 04.1 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,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.62 00:18:15.79 +49:56:31.0
117.47398 -12.57791 galactic Cas Second-epoch detections are separated by 5.1" and 5.6 pix
The object was found in VSX13" Gaia DR3 394504879424744704
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.850 G 14.880 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 00:18:15.79 +49:56:31.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:18:15.79 +49:56:31.0: 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 13.2885* 00 18 15.79 +49 56 31.0 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 394504879424744704,2461234.7885,12.62,0.05,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
Gaia DR3 394504879424744704 20260713.2885 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 13.2885 2461234.7885 12.68 00:24:29.14 +53:23:18.7
118.86622 -9.27032 galactic Cas Second-epoch detections are separated by 4.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:29.14 +53:23:18.7 (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 00:24:29.14 +53:23:18.7: 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 00:24:29.14 +53:23:18.7: 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 13.2885* 00 24 29.14 +53 23 18.7 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,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.65 00:25:28.88 +50:20:21.6
118.69789 -12.31890 galactic Cas Second-epoch detections are separated by 4.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:28.88 +50:20:21.6 (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 00:25:28.88 +50:20:21.6: 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 00:25:28.88 +50:20:21.6: 13.40 +/- 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 13.2885* 00 25 28.88 +50 20 21.6 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,2461234.7885,12.65,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.67 00:22:29.93 +51:14:18.7
118.31892 -11.37383 galactic Cas Second-epoch detections are separated by 1.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:29.93 +51:14:18.7 (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 00:22:29.93 +51:14:18.7: 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 00:22:29.93 +51:14:18.7: 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 13.2885* 00 22 29.93 +51 14 18.7 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,2461234.7885,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.82 00:27:53.14 +51:36:40.1
119.20981 -11.09032 galactic Cas Second-epoch detections are separated by 4.4" and 5.8 pix
The object was found in VSX18" Gaia DR3 418846314517875584
Type: ROT
# Max. Min./Amp. JD0 Period
16.120 G 16.170 G K
ATTENTION: measured mag 12.82 is 3.3 mag brighter than the VSX record maximum brightness 16.12 - 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 00:27:53.14 +51:36:40.1: 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 00:27:53.14 +51:36:40.1: 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 13.2885* 00 27 53.14 +51 36 40.1 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 418846314517875584,2461234.7885,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 418846314517875584 20260713.2885 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.71 00:25:40.54 +49:43:18.4
118.66471 -12.93640 galactic Cas Second-epoch detections are separated by 7.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:40.54 +49:43:18.4 (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 00:25:40.54 +49:43:18.4: 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 00:25:40.54 +49:43:18.4: 13.40 +/- 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 13.2885* 00 25 40.54 +49 43 18.4 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,2461234.7885,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.63 00:27:06.84 +53:36:16.6
119.28219 -9.09468 galactic Cas Second-epoch detections are separated by 2.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:06.84 +53:36:16.6 (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 00:27:06.84 +53:36:16.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:06.84 +53:36:16.6: 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 13.2885* 00 27 06.84 +53 36 16.6 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,2461234.7885,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.55 00:25:59.87 +50:55:09.0
118.84157 -11.75043 galactic Cas Second-epoch detections are separated by 6.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:59.87 +50:55:09.0 (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 00:25:59.87 +50:55:09.0: 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 00:25:59.87 +50:55:09.0: 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 13.2885* 00 25 59.87 +50 55 09.0 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,2461234.7885,12.55,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.72 00:18:39.34 +50:08:44.0
117.56523 -12.38428 galactic Cas Second-epoch detections are separated by 7.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:39.34 +50:08:44.0 (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 00:18:39.34 +50:08:44.0: 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 00:18:39.34 +50:08:44.0: 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 13.2885* 00 18 39.34 +50 08 44.0 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,2461234.7885,12.72,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.60 00:25:00.01 +56:14:23.1
119.24123 -6.44243 galactic Cas Second-epoch detections are separated by 0.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:00.01 +56:14:23.1 (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 00:25:00.01 +56:14:23.1: 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 00:25:00.01 +56:14:23.1: 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 13.2885* 00 25 00.01 +56 14 23.1 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,2461234.7885,12.60,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.60 00:27:18.50 +51:50:42.3
119.14158 -10.84900 galactic Cas Second-epoch detections are separated by 5.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.8237+51.8379 | 00:27:18.50 +51:50:42.3 (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 00:27:18.50 +51:50:42.3: 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 00:27:18.50 +51:50:42.3: 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 13.2885* 00 27 18.50 +51 50 42.3 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 J006.8237+51.8379,2461234.7885,12.60,0.05,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
ATO J006.8237+51.8379 20260713.2885 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 13.2885 2461234.7885 12.87 00:27:32.04 +49:53:18.8
118.98766 -12.80004 galactic Cas Second-epoch detections are separated by 6.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:32.04 +49:53:18.8 (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 00:27:32.04 +49:53:18.8: 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 00:27:32.04 +49:53:18.8: 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 13.2885* 00 27 32.04 +49 53 18.8 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,2461234.7885,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.87CV 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 13.2885 2461234.7885 12.54 00:29:52.44 +53:42:26.9
119.70398 -9.02907 galactic Cas Second-epoch detections are separated by 5.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:29:52.44 +53:42:26.9 (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 00:29:52.44 +53:42:26.9: 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 00:29:52.44 +53:42:26.9: 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 13.2885* 00 29 52.44 +53 42 26.9 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
target,2461234.7885,12.54,0.05,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 20260713.2885 12.54CV 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 13.2885 2461234.7885 12.73 00:26:06.36 +49:46:55.2
118.74193 -12.88355 galactic Cas Second-epoch detections are separated by 8.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:06.36 +49:46:55.2 (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 00:26:06.36 +49:46:55.2: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:06.36 +49:46:55.2: 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 13.2885* 00 26 06.36 +49 46 55.2 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,2461234.7885,12.73,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.56 00:12:49.81 +56:38:44.7
117.61515 -5.82692 galactic Cas Second-epoch detections are separated by 4.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J003.2378+56.6346 | 00:12:54.68 +56:38:24.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:12:49.81 +56:38:44.7: 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 00:12:49.81 +56:38:44.7: 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 13.2885* 00 12 49.81 +56 38 44.7 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 J003.2378+56.6346,2461234.7885,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.2378+56.6346 20260713.2885 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.68 00:20:54.83 +52:26:46.7
118.21552 -10.14569 galactic Cas Second-epoch detections are separated by 2.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:20:54.83 +52:26:46.7 (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 00:20:54.83 +52:26:46.7: 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 00:20:54.83 +52:26:46.7: 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 13.2885* 00 20 54.83 +52 26 46.7 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,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.75 00:28:05.07 +52:23:38.9
119.31455 -10.31351 galactic Cas Second-epoch detections are separated by 3.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:05.07 +52:23:38.9 (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 00:28:05.07 +52:23:38.9: 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 00:28:05.07 +52:23:38.9: 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 13.2885* 00 28 05.07 +52 23 38.9 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,2461234.7885,12.75,0.05,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
target 20260713.2885 12.75CV 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 13.2885 2461234.7885 12.88 00:12:11.56 +50:01:07.2
116.49611 -12.36203 galactic Cas Second-epoch detections are separated by 8.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:12:11.56 +50:01:07.2 (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 00:12:11.56 +50:01:07.2: 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 00:12:11.56 +50:01:07.2: 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 13.2885* 00 12 11.56 +50 01 07.2 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,2461234.7885,12.88,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.76 00:24:09.96 +50:15:32.5
118.47538 -12.37659 galactic Cas Second-epoch detections are separated by 4.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 394659154649246080 | 00:24:11.79 +50:15:54.9 (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 00:24:09.96 +50:15:32.5: 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 00:24:09.96 +50:15:32.5: 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 13.2885* 00 24 09.96 +50 15 32.5 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 394659154649246080,2461234.7885,12.76,0.05,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
Gaia DR3 394659154649246080 20260713.2885 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 13.2885 2461234.7885 12.86 00:26:27.67 +52:48:18.2
119.10502 -9.88100 galactic Cas Second-epoch detections are separated by 3.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:27.67 +52:48:18.2 (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 00:26:27.67 +52:48:18.2: 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 00:26:27.67 +52:48:18.2: 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 13.2885* 00 26 27.67 +52 48 18.2 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,2461234.7885,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.71 00:19:47.94 +49:56:35.6
117.72524 -12.60840 galactic Cas Second-epoch detections are separated by 7.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:47.94 +49:56:35.6 (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 00:19:47.94 +49:56:35.6: 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 00:19:47.94 +49:56:35.6: 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 13.2885* 00 19 47.94 +49 56 35.6 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,2461234.7885,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.79 00:26:28.07 +52:02:02.1
119.02897 -10.64850 galactic Cas Second-epoch detections are separated by 2.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:28.07 +52:02:02.1 (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 00:26:28.07 +52:02:02.1: 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 00:26:28.07 +52:02:02.1: 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 13.2885* 00 26 28.07 +52 02 02.1 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,2461234.7885,12.79,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.75 00:28:26.64 +52:38:28.9
119.39282 -10.07231 galactic Cas Second-epoch detections are separated by 3.4" and 5.7 pix
The object was found in VSX18" Gaia DR3 419019758178266496
Type: ROT
# Max. Min./Amp. JD0 Period
16.710 G 16.780 G K
ATTENTION: measured mag 12.75 is 4.0 mag brighter than the VSX record maximum brightness 16.71 - 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 00:28:26.64 +52:38:28.9: 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 00:28:26.64 +52:38:28.9: 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 13.2885* 00 28 26.64 +52 38 28.9 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 419019758178266496,2461234.7885,12.75,0.05,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
Gaia DR3 419019758178266496 20260713.2885 12.75CV 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 13.2885 2461234.7885 12.66 00:27:12.85 +50:07:02.8
118.95765 -12.56729 galactic Cas Second-epoch detections are separated by 6.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:12.85 +50:07:02.8 (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 00:27:12.85 +50:07:02.8: 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 00:27:12.85 +50:07:02.8: 13.40 +/- 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 13.2885* 00 27 12.85 +50 07 02.8 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
target,2461234.7885,12.66,0.05,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
target 20260713.2885 12.66CV 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 13.2885 2461234.7885 12.78 00:20:27.48 +52:05:03.1
118.10061 -10.49670 galactic Cas Second-epoch detections are separated by 1.8" and 5.8 pix
The object was found in VSX22" ZTF J002029.43+520515.8
Type: EW
# Max. Min./Amp. JD0 Period
14.697 r Y 0.643 r 2458437.72670 0.284894000000
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 00:20:27.48 +52:05:03.1: 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 00:20:27.48 +52:05:03.1: 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 13.2885* 00 20 27.48 +52 05 03.1 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
ZTF J002029.43+520515.8,2461234.7885,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J002029.43+520515.8 20260713.2885 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.59 00:28:22.86 +57:29:15.3
119.82444 -5.24498 galactic Cas Second-epoch detections are separated by 4.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421896669015171072 | 00:28:20.98 +57:29:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:22.86 +57:29:15.3: 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 00:28:22.86 +57:29:15.3: 13.36 +/- 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 13.2885* 00 28 22.86 +57 29 15.3 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
Gaia DR3 421896669015171072,2461234.7885,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421896669015171072 20260713.2885 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.79 00:17:23.60 +51:25:21.8
117.53549 -11.09196 galactic Cas Second-epoch detections are separated by 2.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:17:23.60 +51:25:21.8 (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 00:17:23.60 +51:25:21.8: 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 00:17:23.60 +51:25:21.8: 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 13.2885* 00 17 23.60 +51 25 21.8 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,2461234.7885,12.79,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.81 00:26:07.92 +49:44:43.2
118.74243 -12.92045 galactic Cas Second-epoch detections are separated by 7.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.5384+49.7524 | 00:26:07.92 +49:44:43.2 (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 00:26:07.92 +49:44:43.2: 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 00:26:07.92 +49:44:43.2: 13.38 +/- 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 13.2885* 00 26 07.92 +49 44 43.2 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 J006.5384+49.7524,2461234.7885,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.5384+49.7524 20260713.2885 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.70 00:15:59.44 +49:51:23.2
117.09058 -12.61284 galactic Cas Second-epoch detections are separated by 6.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:15:59.44 +49:51:23.2 (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 00:15:59.44 +49:51:23.2: 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 00:15:59.44 +49:51:23.2: 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 13.2885* 00 15 59.44 +49 51 23.2 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,2461234.7885,12.70,0.05,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 20260713.2885 12.70CV 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 13.2885 2461234.7885 12.74 00:27:39.88 +50:01:01.5
119.02159 -12.67408 galactic Cas Second-epoch detections are separated by 8.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.9413+50.0296 | 00:27:43.51 +50:01:22.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8 1952CoRut..32....1H BD+49 95
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:39.88 +50:01:01.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:39.88 +50:01:01.5: 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 13.2885* 00 27 39.88 +50 01 01.5 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 J006.9413+50.0296,2461234.7885,12.74,0.05,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
ATO J006.9413+50.0296 20260713.2885 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 13.2885 2461234.7885 12.64 00:28:44.79 +55:16:06.5
119.67589 -7.45976 galactic Cas Second-epoch detections are separated by 6.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 421150955312416768 | 00:28:42.64 +55:16:37.4 (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 00:28:44.79 +55:16:06.5: 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 00:28:44.79 +55:16:06.5: 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 13.2885* 00 28 44.79 +55 16 06.5 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 421150955312416768,2461234.7885,12.64,0.05,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
Gaia DR3 421150955312416768 20260713.2885 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 13.2885 2461234.7885 12.49 23:54:55.73 +56:31:16.7
115.15821 -5.49514 galactic Cas Second-epoch detections are separated by 7.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J235455.23+563033.9 | 23:54:55.23 +56:30:33.9 (Gaia DR3) | SR (local) | 31.020000000000 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:54:55.73 +56:31:16.7: 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 23:54:55.73 +56:31:16.7: 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 13.2885* 23 54 55.73 +56 31 16.7 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
ASASSN-V J235455.23+563033.9,2461234.7885,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J235455.23+563033.9 20260713.2885 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.73 00:12:35.21 +52:01:41.7
116.87415 -10.38594 galactic Cas Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:12:35.21 +52:01:41.7 (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 00:12:35.21 +52:01:41.7: 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 00:12:35.21 +52:01:41.7: 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 13.2885* 00 12 35.21 +52 01 41.7 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,2461234.7885,12.73,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.69 00:27:47.97 +52:08:25.3
119.24651 -10.56216 galactic Cas Second-epoch detections are separated by 3.7" and 5.7 pix
The object was found in VSX23" Gaia DR3 418977152104987776
Type: ROT
# Max. Min./Amp. JD0 Period
17.050 G 17.110 G K
ATTENTION: measured mag 12.69 is 4.4 mag brighter than the VSX record maximum brightness 17.05 - 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 00:27:47.97 +52:08:25.3: 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 00:27:47.97 +52:08:25.3: 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 13.2885* 00 27 47.97 +52 08 25.3 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
Gaia DR3 418977152104987776,2461234.7885,12.69,0.05,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 418977152104987776 20260713.2885 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 13.2885 2461234.7885 12.72 00:25:14.90 +49:51:28.7
118.60876 -12.79381 galactic Cas Second-epoch detections are separated by 5.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:14.90 +49:51:28.7 (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 00:25:14.90 +49:51:28.7: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:14.90 +49:51:28.7: 13.36 +/- 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 13.2885* 00 25 14.90 +49 51 28.7 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,2461234.7885,12.72,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.68 00:20:08.60 +53:27:53.1
118.22407 -9.12070 galactic Cas Second-epoch detections are separated by 4.2" and 5.3 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 | 00:20:08.60 +53:27:53.1 (user input) | T | P | (position from user input) J-Ks=0.477+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:20:08.60 +53:27:53.1: 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 00:20:08.60 +53:27:53.1: 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 13.2885* 00 20 08.60 +53 27 53.1 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,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.80 00:30:07.09 +56:57:05.6
120.01324 -5.79933 galactic Cas Second-epoch detections are separated by 3.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:30:07.09 +56:57:05.6 (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 00:30:07.09 +56:57:05.6: 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 00:30:07.09 +56:57:05.6: 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 13.2885* 00 30 07.09 +56 57 05.6 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,2461234.7885,12.80,0.05,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 20260713.2885 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.62 00:19:42.19 +52:22:46.0
118.02105 -10.18945 galactic Cas Second-epoch detections are separated by 4.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.9416+52.3792 | 00:19:42.19 +52:22:46.0 (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 00:19:42.19 +52:22:46.0: 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 00:19:42.19 +52:22:46.0: 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 13.2885* 00 19 42.19 +52 22 46.0 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 J004.9416+52.3792,2461234.7885,12.62,0.05,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
ATO J004.9416+52.3792 20260713.2885 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 13.2885 2461234.7885 12.80 00:26:51.01 +49:46:16.4
118.86347 -12.90620 galactic Cas Second-epoch detections are separated by 4.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:51.01 +49:46:16.4 (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 00:26:51.01 +49:46:16.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:51.01 +49:46:16.4: 13.38 +/- 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 13.2885* 00 26 51.01 +49 46 16.4 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,2461234.7885,12.80,0.05,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 20260713.2885 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.72 00:21:27.38 +50:49:24.9
118.10343 -11.76687 galactic Cas Second-epoch detections are separated by 2.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:27.38 +50:49:24.9 (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 00:21:27.38 +50:49:24.9: 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 00:21:27.38 +50:49:24.9: 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 13.2885* 00 21 27.38 +50 49 24.9 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,2461234.7885,12.72,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.84 00:22:10.45 +52:54:58.0
118.46415 -9.70159 galactic Cas Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:10.45 +52:54:58.0 (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 00:22:10.45 +52:54:58.0: 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 00:22:10.45 +52:54:58.0: 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 13.2885* 00 22 10.45 +52 54 58.0 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,2461234.7885,12.84,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.76 00:22:17.09 +52:50:24.0
118.47211 -9.77912 galactic Cas Second-epoch detections are separated by 1.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:17.09 +52:50:24.0 (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 00:22:17.09 +52:50:24.0: 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 00:22:17.09 +52:50:24.0: 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 13.2885* 00 22 17.09 +52 50 24.0 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,2461234.7885,12.76,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.72 00:26:21.17 +50:40:28.0
118.87358 -11.99953 galactic Cas Second-epoch detections are separated by 5.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.5748+50.6671 | 00:26:21.17 +50:40:28.0 (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 00:26:21.17 +50:40:28.0: 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 00:26:21.17 +50:40:28.0: 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 13.2885* 00 26 21.17 +50 40 28.0 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
ATO J006.5748+50.6671,2461234.7885,12.72,0.05,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 J006.5748+50.6671 20260713.2885 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 13.2885 2461234.7885 12.71 00:26:48.60 +52:36:36.7
119.13911 -10.08009 galactic Cas Second-epoch detections are separated by 5.8" and 6.1 pix
The object was found in VSX23" Gaia DR3 419028283695520768
Type: ROT
# Max. Min./Amp. JD0 Period
16.010 G 16.070 G G
ATTENTION: measured mag 12.71 is 3.3 mag brighter than the VSX record maximum brightness 16.01 - 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 00:26:48.60 +52:36:36.7: 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 00:26:48.60 +52:36:36.7: 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 13.2885* 00 26 48.60 +52 36 36.7 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 419028283695520768,2461234.7885,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419028283695520768 20260713.2885 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.80 00:29:07.59 +52:19:12.8
119.46887 -10.40144 galactic Cas Second-epoch detections are separated by 4.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:29:07.59 +52:19:12.8 (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 00:29:07.59 +52:19:12.8: 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 00:29:07.59 +52:19:12.8: 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 13.2885* 00 29 07.59 +52 19 12.8 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,2461234.7885,12.80,0.05,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 20260713.2885 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.79 00:21:08.05 +51:41:04.5
118.15692 -10.90599 galactic Cas Second-epoch detections are separated by 2.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:08.05 +51:41:04.5 (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 00:21:08.05 +51:41:04.5: 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 00:21:08.05 +51:41:04.5: 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 13.2885* 00 21 08.05 +51 41 04.5 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,2461234.7885,12.79,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.62 00:24:02.78 +55:28:19.1
119.02597 -7.19190 galactic Cas Second-epoch detections are separated by 3.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:02.78 +55:28:19.1 (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 00:24:02.78 +55:28:19.1: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:24:02.78 +55:28:19.1: 13.38 +/- 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 13.2885* 00 24 02.78 +55 28 19.1 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,2461234.7885,12.62,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.77 00:26:00.38 +51:13:40.9
118.87465 -11.44327 galactic Cas Second-epoch detections are separated by 0.7" and 5.2 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 | 00:26:00.38 +51:13:40.9 (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 00:26:00.38 +51:13:40.9: 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 00:26:00.38 +51:13:40.9: 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 13.2885* 00 26 00.38 +51 13 40.9 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,2461234.7885,12.77,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.85 00:27:11.52 +51:41:47.4
119.10889 -10.99518 galactic Cas Second-epoch detections are separated by 3.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:11.52 +51:41:47.4 (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 00:27:11.52 +51:41:47.4: 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 00:27:11.52 +51:41:47.4: 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 13.2885* 00 27 11.52 +51 41 47.4 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,2461234.7885,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.65 00:27:12.40 +54:18:54.6
119.36437 -8.38865 galactic Cas Second-epoch detections are separated by 4.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:12.40 +54:18:54.6 (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 00:27:12.40 +54:18:54.6: 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 00:27:12.40 +54:18:54.6: 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 13.2885* 00 27 12.40 +54 18 54.6 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,2461234.7885,12.65,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.87 00:24:24.90 +52:58:26.1
118.81099 -9.68148 galactic Cas Second-epoch detections are separated by 2.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:24.90 +52:58:26.1 (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 00:24:24.90 +52:58:26.1: 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 00:24:24.90 +52:58:26.1: 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 13.2885* 00 24 24.90 +52 58 26.1 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,2461234.7885,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.87CV 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 13.2885 2461234.7885 12.67 00:19:04.80 +51:18:58.4
117.78728 -11.23201 galactic Cas Second-epoch detections are separated by 3.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:04.80 +51:18:58.4 (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 00:19:04.80 +51:18:58.4: 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 00:19:04.80 +51:18:58.4: 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 13.2885* 00 19 04.80 +51 18 58.4 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,2461234.7885,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.76 00:18:44.49 +51:17:52.0
117.73138 -11.24352 galactic Cas Second-epoch detections are separated by 1.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:18:44.49 +51:17:52.0 (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 00:18:44.49 +51:17:52.0: 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 00:18:44.49 +51:17:52.0: 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 13.2885* 00 18 44.49 +51 17 52.0 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,2461234.7885,12.76,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.71 00:28:50.00 +52:17:32.3
119.42097 -10.42528 galactic Cas Second-epoch detections are separated by 3.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:28:50.00 +52:17:32.3 (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 00:28:50.00 +52:17:32.3: 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 00:28:50.00 +52:17:32.3: 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 13.2885* 00 28 50.00 +52 17 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,2461234.7885,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.75 00:25:12.60 +56:31:45.4
119.30019 -6.15741 galactic Cas Second-epoch detections are separated by 6.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:12.60 +56:31:45.4 (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 00:25:12.60 +56:31:45.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:12.60 +56:31:45.4: 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 13.2885* 00 25 12.60 +56 31 45.4 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,2461234.7885,12.75,0.05,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
target 20260713.2885 12.75CV 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 13.2885 2461234.7885 12.68 00:15:49.15 +50:44:30.1
117.19017 -11.73253 galactic Cas Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:15:49.15 +50:44:30.1 (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 00:15:49.15 +50:44:30.1: 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 00:15:49.15 +50:44:30.1: 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 13.2885* 00 15 49.15 +50 44 30.1 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,2461234.7885,12.68,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.63 00:17:13.10 +57:50:20.7
118.37475 -4.72956 galactic Cas Second-epoch detections are separated by 7.0" and 6.3 pix
The object was found in VSX 3" Gaia DR3 422061114723435008
Type: ROT
# Max. Min./Amp. JD0 Period
14.500 G 14.540 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 00:17:13.10 +57:50:20.7: 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 00:17:13.10 +57:50:20.7: 13.36 +/- 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 13.2885* 00 17 13.10 +57 50 20.7 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
Gaia DR3 422061114723435008,2461234.7885,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 422061114723435008 20260713.2885 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.72 00:26:45.25 +51:29:25.7
119.01963 -11.19367 galactic Cas Second-epoch detections are separated by 4.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 418841779034047616 | 00:26:44.88 +51:30:08.8 (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 00:26:45.25 +51:29:25.7: 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 00:26:45.25 +51:29:25.7: 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 13.2885* 00 26 45.25 +51 29 25.7 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 418841779034047616,2461234.7885,12.72,0.05,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
Gaia DR3 418841779034047616 20260713.2885 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 13.2885 2461234.7885 12.77 00:27:23.78 +54:00:55.1
119.36363 -8.68979 galactic Cas Second-epoch detections are separated by 3.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:23.78 +54:00:55.1 (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 00:27:23.78 +54:00:55.1: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:23.78 +54:00:55.1: 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 13.2885* 00 27 23.78 +54 00 55.1 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,2461234.7885,12.77,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.59 23:23:39.95 +49:26:42.9
108.60339 -10.96902 galactic And Second-epoch detections are separated by 5.6" and 5.7 pix
The object was found in VSX15" Gaia DR3 1943061454032400384
Type: ROT
# Max. Min./Amp. JD0 Period
13.960 G 14.010 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 23:23:39.95 +49:26:42.9: 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 23:23:39.95 +49:26:42.9: 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 13.2885* 23 23 39.95 +49 26 42.9 12.6 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
Gaia DR3 1943061454032400384,2461234.7885,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943061454032400384 20260713.2885 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.77 00:25:18.10 +57:04:42.7
119.36905 -5.61231 galactic Cas Second-epoch detections are separated by 8.3" and 5.1 pix
The object was found in VSX19" Gaia DR3 421776890966957184
Type: ROT
# Max. Min./Amp. JD0 Period
16.250 G 16.290 G K
ATTENTION: measured mag 12.77 is 3.5 mag brighter than the VSX record maximum brightness 16.25 - 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 00:25:18.10 +57:04:42.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:18.10 +57:04:42.7: 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 13.2885* 00 25 18.10 +57 04 42.7 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 421776890966957184,2461234.7885,12.77,0.05,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 421776890966957184 20260713.2885 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 13.2885 2461234.7885 12.79 00:17:18.60 +57:02:33.1
118.28086 -5.52071 galactic Cas Second-epoch detections are separated by 2.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:17:18.60 +57:02:33.1 (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 00:17:18.60 +57:02:33.1: 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 00:17:18.60 +57:02:33.1: 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 13.2885* 00 17 18.60 +57 02 33.1 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,2461234.7885,12.79,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.89 00:27:57.87 +53:27:54.7
119.39638 -9.24534 galactic Cas Second-epoch detections are separated by 0.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:57.87 +53:27:54.7 (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 00:27:57.87 +53:27:54.7: 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 00:27:57.87 +53:27:54.7: 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 13.2885* 00 27 57.87 +53 27 54.7 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,2461234.7885,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.86 00:26:35.77 +52:23:53.9
119.08523 -10.28780 galactic Cas Second-epoch detections are separated by 2.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.6387+52.4060 | 00:26:35.77 +52:23:53.9 (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 00:26:35.77 +52:23:53.9: 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 00:26:35.77 +52:23:53.9: 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 13.2885* 00 26 35.77 +52 23 53.9 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
ATO J006.6387+52.4060,2461234.7885,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.6387+52.4060 20260713.2885 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.82 00:16:16.13 +56:02:21.4
118.00190 -6.49546 galactic Cas Second-epoch detections are separated by 8.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J004.0869+56.0441 | 00:16:16.13 +56:02:21.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:16:16.13 +56:02:21.4: 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 00:16:16.13 +56:02:21.4: 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 13.2885* 00 16 16.13 +56 02 21.4 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
ATO J004.0869+56.0441,2461234.7885,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.0869+56.0441 20260713.2885 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.66 00:30:18.77 +56:07:42.4
119.97160 -6.62183 galactic Cas Second-epoch detections are separated by 8.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.5923+56.1336 | 00:30:18.77 +56:07:42.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.549+/-0.137 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:18.77 +56:07:42.4: 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 00:30:18.77 +56:07:42.4: 13.36 +/- 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 13.2885* 00 30 18.77 +56 07 42.4 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 J007.5923+56.1336,2461234.7885,12.66,0.05,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
ATO J007.5923+56.1336 20260713.2885 12.66CV 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 13.2885 2461234.7885 12.86 00:28:36.78 +57:23:02.9
119.84639 -5.35080 galactic Cas Second-epoch detections are separated by 2.6" and 6.0 pix
The object was found in VSX11" Gaia DR3 421825372555240320
Type: S
# Max. Min./Amp. JD0 Period
15.420 G 16.100 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 00:28:36.78 +57:23:02.9: 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 00:28:36.78 +57:23:02.9: 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 13.2885* 00 28 36.78 +57 23 02.9 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
Gaia DR3 421825372555240320,2461234.7885,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421825372555240320 20260713.2885 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.80 00:15:55.99 +51:39:55.6
117.34031 -10.82042 galactic Cas Second-epoch detections are separated by 1.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:15:55.99 +51:39:55.6 (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 00:15:55.99 +51:39:55.6: 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 00:15:55.99 +51:39:55.6: 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 13.2885* 00 15 55.99 +51 39 55.6 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,2461234.7885,12.80,0.05,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 20260713.2885 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.80 00:24:40.29 +55:59:40.1
119.16975 -6.68163 galactic Cas Second-epoch detections are separated by 2.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.1832+55.9950 | 00:24:40.29 +55:59:40.1 (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 00:24:40.29 +55:59:40.1: 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 00:24:40.29 +55:59:40.1: 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 13.2885* 00 24 40.29 +55 59 40.1 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 J006.1832+55.9950,2461234.7885,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.1832+55.9950 20260713.2885 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.73 00:30:54.29 +55:16:20.2
119.98514 -7.48195 galactic Cas Second-epoch detections are separated by 6.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:30:54.29 +55:16:20.2 (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 00:30:54.29 +55:16:20.2: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:54.29 +55:16:20.2: 12.98 +/- 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 13.2885* 00 30 54.29 +55 16 20.2 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,2461234.7885,12.73,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.74 00:10:32.47 +52:19:31.2
116.60667 -10.04343 galactic Cas Second-epoch detections are separated by 1.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J002.6587+52.3113 | 00:10:34.23 +52:18:59.9 (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 00:10:32.47 +52:19:31.2: 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 00:10:32.47 +52:19:31.2: 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 13.2885* 00 10 32.47 +52 19 31.2 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 J002.6587+52.3113,2461234.7885,12.74,0.05,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
ATO J002.6587+52.3113 20260713.2885 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 13.2885 2461234.7885 12.65 00:13:38.27 +54:57:36.2
117.47580 -7.51075 galactic Cas Second-epoch detections are separated by 3.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 420565057353289216 | 00:13:40.42 +54:57:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F4 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:13:38.27 +54:57:36.2: 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 00:13:38.27 +54:57:36.2: 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 13.2885* 00 13 38.27 +54 57 36.2 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 420565057353289216,2461234.7885,12.65,0.05,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
Gaia DR3 420565057353289216 20260713.2885 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 13.2885 2461234.7885 12.58 00:21:43.15 +54:48:13.6
118.61745 -7.81882 galactic Cas Second-epoch detections are separated by 3.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:21:43.15 +54:48:13.6 (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 00:21:43.15 +54:48:13.6: 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 00:21:43.15 +54:48:13.6: 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 13.2885* 00 21 43.15 +54 48 13.6 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,2461234.7885,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260713.2885 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 13.2885 2461234.7885 12.82 00:16:25.43 +53:02:33.7
117.60954 -9.46683 galactic Cas Second-epoch detections are separated by 4.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:16:25.43 +53:02:33.7 (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 00:16:25.43 +53:02:33.7: 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 00:16:25.43 +53:02:33.7: 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 13.2885* 00 16 25.43 +53 02 33.7 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,2461234.7885,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.79 00:30:41.22 +55:28:16.4
119.97023 -7.28115 galactic Cas Second-epoch detections are separated by 5.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J007.6745+55.4710 | 00:30:41.22 +55:28:16.4 (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 00:30:41.22 +55:28:16.4: 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 00:30:41.22 +55:28:16.4: 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 13.2885* 00 30 41.22 +55 28 16.4 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
ATO J007.6745+55.4710,2461234.7885,12.79,0.05,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
ATO J007.6745+55.4710 20260713.2885 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 13.2885 2461234.7885 12.63 23:55:17.80 +56:36:24.9
115.22660 -5.42260 galactic Cas Second-epoch detections are separated by 8.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:55:17.80 +56:36:24.9 (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 23:55:17.80 +56:36:24.9: 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 23:55:17.80 +56:36:24.9: 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 13.2885* 23 55 17.80 +56 36 24.9 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,2461234.7885,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.71 00:29:26.67 +55:24:39.1
119.78813 -7.32658 galactic Cas Second-epoch detections are separated by 5.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:29:26.67 +55:24:39.1 (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 00:29:26.67 +55:24:39.1: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:26.67 +55:24:39.1: 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 13.2885* 00 29 26.67 +55 24 39.1 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,2461234.7885,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.88 00:19:51.26 +57:01:50.4
118.62421 -5.57668 galactic Cas Second-epoch detections are separated by 4.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:51.26 +57:01:50.4 (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 00:19:51.26 +57:01:50.4: 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 00:19:51.26 +57:01:50.4: 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 13.2885* 00 19 51.26 +57 01 50.4 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,2461234.7885,12.88,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.82 23:57:06.71 +51:17:45.6
114.33862 -10.66705 galactic Cas Second-epoch detections are separated by 4.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:57:06.71 +51:17:45.6 (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 23:57:06.71 +51:17:45.6: 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 23:57:06.71 +51:17:45.6: 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 13.2885* 23 57 06.71 +51 17 45.6 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,2461234.7885,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.61 00:10:31.73 +53:26:21.2
116.78572 -8.94363 galactic Cas Second-epoch detections are separated by 5.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:10:31.73 +53:26:21.2 (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 00:10:31.73 +53:26:21.2: 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 00:10:31.73 +53:26:21.2: 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 13.2885* 00 10 31.73 +53 26 21.2 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,2461234.7885,12.61,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.75 00:12:02.75 +54:10:32.6
117.12627 -8.25139 galactic Cas Second-epoch detections are separated by 8.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:12:02.75 +54:10:32.6 (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 00:12:02.75 +54:10:32.6: 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 00:12:02.75 +54:10:32.6: 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 13.2885* 00 12 02.75 +54 10 32.6 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,2461234.7885,12.75,0.05,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
target 20260713.2885 12.75CV 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 13.2885 2461234.7885 12.73 00:07:57.79 +53:09:53.4
116.35707 -9.15102 galactic Cas Second-epoch detections are separated by 3.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:07:57.79 +53:09:53.4 (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 00:07:57.79 +53:09:53.4: 13.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:07:57.79 +53:09:53.4: 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 13.2885* 00 07 57.79 +53 09 53.4 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,2461234.7885,12.73,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.84 00:17:14.21 +56:19:32.5
118.17509 -6.22985 galactic Cas Second-epoch detections are separated by 7.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:17:14.21 +56:19:32.5 (user input) | T | P | (position from user input) 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 00:17:14.21 +56:19:32.5: 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 00:17:14.21 +56:19:32.5: 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 13.2885* 00 17 14.21 +56 19 32.5 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,2461234.7885,12.84,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.71 00:24:47.09 +56:08:45.9
119.20148 -6.53249 galactic Cas Second-epoch detections are separated by 3.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:47.09 +56:08:45.9 (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 00:24:47.09 +56:08:45.9: 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 00:24:47.09 +56:08:45.9: 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 13.2885* 00 24 47.09 +56 08 45.9 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,2461234.7885,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.70 00:30:39.20 +57:46:18.9
120.15305 -4.98764 galactic Cas Second-epoch detections are separated by 6.4" and 5.7 pix
The object was found in VSX 7" Gaia DR3 427862584745469568
Type: ROT
# Max. Min./Amp. JD0 Period
14.190 G 14.250 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 00:30:39.20 +57:46:18.9: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:39.20 +57:46:18.9: 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 13.2885* 00 30 39.20 +57 46 18.9 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 427862584745469568,2461234.7885,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427862584745469568 20260713.2885 12.70CV 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 13.2885 2461234.7885 12.70 23:29:35.40 +53:27:37.2
110.81426 -7.47476 galactic Cas Second-epoch detections are separated by 8.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1992746838299918720 | 23:29:35.59 +53:28:22.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:35.40 +53:27:37.2: 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 23:29:35.40 +53:27:37.2: 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 13.2885* 23 29 35.40 +53 27 37.2 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
Large-amplitude variable Gaia DR2 1992746838299918720,2461234.7885,12.70,0.05,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
Large-amplitude variable Gaia DR2 1992746838299918720 20260713.2885 12.70CV 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 13.2885 2461234.7885 12.63 23:45:36.35 +50:06:48.3
112.25162 -11.38820 galactic Cas Second-epoch detections are separated by 7.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:45:36.35 +50:06:48.3 (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 23:45:36.35 +50:06:48.3: 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 23:45:36.35 +50:06:48.3: 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 13.2885* 23 45 36.35 +50 06 48.3 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,2461234.7885,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.79 23:32:07.61 +51:53:29.5
110.69269 -9.08550 galactic Cas Second-epoch detections are separated by 2.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:32:07.61 +51:53:29.5 (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 23:32:07.61 +51:53:29.5: 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 23:32:07.61 +51:53:29.5: 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 13.2885* 23 32 07.61 +51 53 29.5 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,2461234.7885,12.79,0.05,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 20260713.2885 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 13.2885 2461234.7885 12.69 23:41:05.57 +55:10:25.8
112.93432 -6.32659 galactic Cas Second-epoch detections are separated by 8.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:41:05.57 +55:10:25.8 (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 23:41:05.57 +55:10:25.8: 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 23:41:05.57 +55:10:25.8: 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 13.2885* 23 41 05.57 +55 10 25.8 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
target,2461234.7885,12.69,0.05,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
target 20260713.2885 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 13.2885 2461234.7885 12.67 23:23:00.98 +49:26:22.2
108.50027 -10.93854 galactic And Second-epoch detections are separated by 5.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:23:00.98 +49:26:22.2 (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 23:23:00.98 +49:26:22.2: 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 23:23:00.98 +49:26:22.2: 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 13.2885* 23 23 00.98 +49 26 22.2 12.7 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
target,2461234.7885,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 12.92 23:16:55.27 +56:25:16.9
110.09095 -4.07563 galactic Cas Second-epoch detections are separated by 1.4" 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 | target | 23:16:55.27 +56:25:16.9 (user input) | T | P | (position from user input) J-Ks=1.133+/- (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:16:55.27 +56:25:16.9: 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 23:16:55.27 +56:25:16.9: 13.40 +/- 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 13.2885* 23 16 55.27 +56 25 16.9 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,2461234.7885,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260713.2885 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 13.2885 2461234.7885 9.58 23:11:50.98 +56:02:39.9
109.29507 -4.16791 galactic Cas Second-epoch detections are separated by 3.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2008809839892102016 | 23:11:49.19 +56:02:21.1 (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 23:11:50.98 +56:02:39.9: 13.14 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:11:50.98 +56:02:39.9: 12.92 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 23 11 50.98 +56 02 39.9 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2008809839892102016,2461234.7885,9.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2008809839892102016 20260713.2885 9.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 13.2885 2461234.7885 11.93 00:25:59.25 +53:55:33.9
119.14626 -8.75849 galactic Cas Second-epoch detections are separated by 2.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:59.25 +53:55:33.9 (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 00:25:59.25 +53:55:33.9: 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 00:25:59.25 +53:55:33.9: 13.44 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 13.2885* 00 25 59.25 +53 55 33.9 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461234.7885,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260713.2885 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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: 2461234.78875032 13.07.2026 06:55:38.028 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 40
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: 140 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): 20703
Objects passed selection criteria: 20686
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 19752.8
Average stars matched: 18516 (93.7388 %)
Memory usage VmPeak: 129688 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Jul 11 21:08:03 CDT 2026
VaST build number 1.0rc89-146-gb95cfcf3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 13 08:43:47 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: 2461234.78875032 13.07.2026 06:55:38.028 /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1101
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: 424 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): 162254
Objects passed selection criteria: 161782
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: 153523
Average stars matched: 142795 (93.0123 %)
Memory usage VmPeak: 1987296 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Jul 11 21:08:03 CDT 2026
VaST build number 1.0rc89-146-gb95cfcf3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 13 09:08:11 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461234.78823116
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_01-54-53_20.00sec_4.90C_LIGHT_0076.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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_01-54-53_20.00sec_4.90C_LIGHT_0076.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
Image size: 927.2'x616.5' 15.5(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: 23:59:51.454 +54:03:03.55 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 23:59:51.454 +54:03:03.55
Angular distance between the image centers 0.0508 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_01-55-38_20.00sec_5.00C_LIGHT_0077.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
Image size: 927.2'x616.6' 15.5(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: 23:59:53.633 +54:03:31.66 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 23:59:53.633 +54:03:31.66
Angular distance between the image centers 0.0557 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 23:59:51.454 +54:03:03.55
Second-epoch second image center 23:59:53.633 +54:03:31.66
Angular distance between the image centers 0.00945 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.b3UHSIXnu3
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.Ul9CLzdpAL
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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits &> /tmp/tmp.9QcmlSzRVm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits &> /tmp/tmp.APDHijcbtx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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 33 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
2.5 pix fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
2.5 pix fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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
14.9 mag. fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
14.9 mag. fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.b3UHSIXnu3 (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_021202_TTUQ2b1x1_3120339_IayKQ02p/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.Ul9CLzdpAL (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_021202_TTUQ2b1x1_3120339_IayKQ02p/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.9QcmlSzRVm (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_021202_TTUQ2b1x1_3120339_IayKQ02p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.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_01-54-53_20.00sec_4.90C_LIGHT_0076.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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.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=2679, bad_region=6065, passed=27496
Got 27496 stars (including 19186 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits.wcscat
util/solve_plate_with_UCAC5 got 27496 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.2'
Seting catalog search parameters based on the expected field of view 927.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012878 (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 0.010302 (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 344.9609 through 0 to 14.9332, gap 14.9332 to 344.9609
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 315 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 218 matched stars entering correct_measured_positions(), 143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 209 matched stars entering correct_measured_positions(), 4574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.99"
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 344.9529 through 0 to 14.9575, gap 14.9575 to 344.9529
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 380 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 310 matched stars entering correct_measured_positions(), 4641 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.94"
Accuracy estimation diagnostic: 308 matched stars entering correct_measured_positions(), 7195 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.08"
Excluding outliers - 308 stars left (next iteration limit 229)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits N_match=308 sigma_overall_arcsec=9.744 sigma_q1_arcsec=31.147 sigma_q2_arcsec=25.306 sigma_q3_arcsec=8.374 sigma_q4_arcsec=7.936 n_q1=33 n_q2=25 n_q3=112 n_q4=138 worst_quadrant_to_overall_ratio=3.196
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.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.APDHijcbtx (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_021202_TTUQ2b1x1_3120339_IayKQ02p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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_01-55-38_20.00sec_5.00C_LIGHT_0077.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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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=2653, bad_region=6081, passed=27402
Got 27402 stars (including 19092 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits.wcscat
util/solve_plate_with_UCAC5 got 27402 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.2'
Seting catalog search parameters based on the expected field of view 927.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012878 (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 0.010302 (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 344.9609 through 0 to 14.9822, gap 14.9822 to 344.9609
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 313 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 219 matched stars entering correct_measured_positions(), 139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 213 matched stars entering correct_measured_positions(), 4697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.24"
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 344.9544 through 0 to 15.0048, gap 15.0048 to 344.9544
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 381 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 313 matched stars entering correct_measured_positions(), 4757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.21"
Accuracy estimation diagnostic: 311 matched stars entering correct_measured_positions(), 7154 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.72"
Excluding outliers - 311 stars left (next iteration limit 234)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits N_match=311 sigma_overall_arcsec=11.436 sigma_q1_arcsec=30.125 sigma_q2_arcsec=24.204 sigma_q3_arcsec=8.441 sigma_q4_arcsec=10.906 n_q1=32 n_q2=24 n_q3=118 n_q4=137 worst_quadrant_to_overall_ratio=2.634
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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_021202_TTUQ2b1x1_3120339_IayKQ02p/fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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_01-54-53_20.00sec_4.90C_LIGHT_0076.fits sigma_overall=9.744 worst_q_ratio=3.196
new2=fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits sigma_overall=11.436 worst_q_ratio=2.634
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_01-54-53_20.00sec_4.90C_LIGHT_0076_astrometric_residuals.png (308 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077_astrometric_residuals.png (311 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.75 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-54-53_20.00sec_4.90C_LIGHT_0076.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-13_CI_Cas-04-Q2b1x1_021202_TTUQ2b1x1_3120339_IayKQ02p/wcs_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077.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 23:46:41.61 +54:28:42.6: 13.43 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:55:31.43 +55:38:22.4: 11.53 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:11:50.17 +56:02:36.5: 14.97 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:18:52.07 +53:18:34.0: 8.87 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:23:39.91 +53:29:32.0: 14.76 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:23:06.20 +51:46:47.4: 15.22 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:43:47.44 +51:12:44.4: 11.55 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:22:00.58 +50:22:27.8: 11.72 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:12:50.87 +57:13:11.0: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:31:49.50 +55:35:28.2: 13.12 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:43:47.44 +51:12:44.4: 11.56 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:39.91 +53:29:32.0: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:46:41.61 +54:28:42.6: 13.46 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:23:06.20 +51:46:47.4: 15.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:55:31.43 +55:38:22.4: 11.55 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:18:52.07 +53:18:34.0: 8.88 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:11:50.17 +56:02:36.5: 14.84 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.23
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Forced photometry reference-image weighted average: 15.22 +/- 0.36
Forced photometry reference-image weighted average: 13.44 +/- 0.05
Forced photometry filter KEPT candidate at 00:23:39.91 +53:29:32.0: ref_mag=14.76 +/- 0.23 new_mean_mag=11.5685 delta=3.19 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:12:50.87 +57:13:11.0: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:22:00.58 +50:22:27.8: 11.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 8.87 +/- 0.00
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Forced photometry filter REJECTED candidate at 23:43:47.44 +51:12:44.4: ref_mag=11.55 +/- 0.01 new_mean_mag=11.4087 delta=0.15 (need > 0.90)
Forced photometry filter KEPT candidate at 00:23:06.20 +51:46:47.4: ref_mag=15.22 +/- 0.36 new_mean_mag=11.6090 delta=3.61 (need > 0.90)
Forced photometry filter KEPT candidate at 23:46:41.61 +54:28:42.6: ref_mag=13.44 +/- 0.05 new_mean_mag=11.6104 delta=1.83 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:18:52.07 +53:18:34.0: ref_mag=8.87 +/- 0.00 new_mean_mag=11.2797 delta=-2.41 (need > 0.90)
Forced photometry reference-image weighted average: 14.90 +/- 0.23
Forced photometry filter REJECTED candidate at 23:55:31.43 +55:38:22.4: ref_mag=11.54 +/- 0.01 new_mean_mag=11.5900 delta=-0.05 (need > 0.90)
Forced photometry filter KEPT candidate at 23:11:50.17 +56:02:36.5: ref_mag=14.90 +/- 0.23 new_mean_mag=11.1731 delta=3.72 (need > 0.90)
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Forced photometry filter REJECTED candidate at 23:22:00.58 +50:22:27.8: ref_mag=11.71 +/- 0.01 new_mean_mag=11.6644 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:31:49.50 +55:35:28.2: 12.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Forced photometry filter KEPT candidate at 23:31:49.50 +55:35:28.2: ref_mag=12.98 +/- 0.03 new_mean_mag=11.6837 delta=1.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:38:04.05 +57:45:23.3: 15.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:32:03.76 +53:56:58.5: 11.84 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:21:27.29 +49:32:31.6: 12.28 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:46:35.12 +54:28:36.8: 14.47 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:38:04.05 +57:45:23.3: 15.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:32:03.76 +53:56:58.5: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter REJECTED candidate at 23:32:03.76 +53:56:58.5: ref_mag=11.77 +/- 0.01 new_mean_mag=11.7160 delta=0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:21:27.29 +49:32:31.6: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.02
Forced photometry filter REJECTED candidate at 23:21:27.29 +49:32:31.6: ref_mag=12.19 +/- 0.02 new_mean_mag=11.7385 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 23:46:35.12 +54:28:36.8: 14.81 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.15
Forced photometry filter KEPT candidate at 23:46:35.12 +54:28:36.8: ref_mag=14.59 +/- 0.15 new_mean_mag=11.7661 delta=2.82 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:19:58.34 +51:55:30.9: 13.73 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:36:38.52 +51:42:55.0: 12.76 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:19:58.34 +51:55:30.9: 13.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.07
Forced photometry filter KEPT candidate at 00:19:58.34 +51:55:30.9: ref_mag=13.69 +/- 0.07 new_mean_mag=11.7828 delta=1.91 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:20.30 +56:49:19.5: 13.97 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:36:38.52 +51:42:55.0: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter KEPT candidate at 23:36:38.52 +51:42:55.0: ref_mag=12.71 +/- 0.02 new_mean_mag=11.7927 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:20.30 +56:49:19.5: 14.08 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.10
Forced photometry filter KEPT candidate at 23:25:20.30 +56:49:19.5: ref_mag=14.02 +/- 0.10 new_mean_mag=11.8203 delta=2.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:38:37.80 +57:12:37.7: 12.58 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:38:37.80 +57:12:37.7: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Forced photometry filter REJECTED candidate at 23:38:37.80 +57:12:37.7: ref_mag=12.52 +/- 0.02 new_mean_mag=11.7706 delta=0.75 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:42:41.43 +51:35:36.2: 11.95 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:42:41.43 +51:35:36.2: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Forced photometry filter REJECTED candidate at 23:42:41.43 +51:35:36.2: ref_mag=11.91 +/- 0.01 new_mean_mag=11.8244 delta=0.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:48:11.47 +57:53:12.0: 13.22 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:48:11.47 +57:53:12.0: 13.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Forced photometry filter KEPT candidate at 23:48:11.47 +57:53:12.0: ref_mag=13.22 +/- 0.04 new_mean_mag=11.8167 delta=1.40 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:45:47.04 +51:21:35.5: 11.80 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:45:47.04 +51:21:35.5: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry filter REJECTED candidate at 23:45:47.04 +51:21:35.5: ref_mag=11.81 +/- 0.01 new_mean_mag=11.8639 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 23:43:48.38 +52:16:10.7: 11.95 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:43:48.38 +52:16:10.7: 11.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Forced photometry filter REJECTED candidate at 23:43:48.38 +52:16:10.7: ref_mag=11.95 +/- 0.01 new_mean_mag=11.8266 delta=0.12 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:30.50 +54:23:42.9: 14.67 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:30.50 +54:23:42.9: 14.26 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.11
Forced photometry filter KEPT candidate at 23:57:30.50 +54:23:42.9: ref_mag=14.40 +/- 0.11 new_mean_mag=11.8613 delta=2.54 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:21:45.74 +54:26:17.6: 13.08 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:16:38.24 +57:25:37.4: 13.01 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:21:45.74 +54:26:17.6: 13.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.04
Forced photometry filter KEPT candidate at 23:21:45.74 +54:26:17.6: ref_mag=13.11 +/- 0.04 new_mean_mag=11.8315 delta=1.28 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:16:38.24 +57:25:37.4: 12.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.03
Forced photometry filter KEPT candidate at 23:16:38.24 +57:25:37.4: ref_mag=12.88 +/- 0.03 new_mean_mag=11.8703 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:41:42.90 +57:35:48.4: 12.36 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:41:42.90 +57:35:48.4: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.02
Forced photometry filter REJECTED candidate at 23:41:42.90 +57:35:48.4: ref_mag=12.27 +/- 0.02 new_mean_mag=11.7952 delta=0.47 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:13:08.93 +56:57:55.6: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:09:29.89 +51:35:56.4: 12.43 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:13:08.93 +56:57:55.6: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:09:29.89 +51:35:56.4: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Forced photometry filter KEPT candidate at 00:09:29.89 +51:35:56.4: ref_mag=12.45 +/- 0.02 new_mean_mag=10.0590 delta=2.39 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out31309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out05724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31391.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 29s
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: 10s
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Considering the candidate 31266_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31266_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31267_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31267_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31271_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31271_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31309_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31309_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
**** FOUND 00:12:50.87 +57:13:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 5.685 422384916598150272 003.21062613641 +57.21831749337 11.4083 10.8817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31316_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31316_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31324_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31324_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31341_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31341_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31343_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31343_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31346_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31346_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31350_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31350_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 31351_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31351_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31354_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31354_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31355_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31355_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
**** FOUND 23:38:04.05 +57:45:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 3.920 1998905477810564480 354.51887023208 +57.75624314601 11.6206 11.2838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31357_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31357_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 31358_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31358_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31361_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31361_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31363_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31363_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 31365_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31365_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31371_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31371_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31372_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31372_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31373_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31373_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31374_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31374_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 31375_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31375_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31376_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31376_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
**** FOUND 23:48:11.47 +57:53:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 2.583 1999071400988590848 357.04886904628 +57.88623442650 11.9634 11.4096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31379_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31379_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31382_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31382_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31385_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31385_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31386_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31386_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31388_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31388_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 31389_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 31389_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 31391_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 31391_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 05724_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 05724_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 17508_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 17508_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 191043_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191043_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 191061_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191061_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 191081_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191081_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (36.1") between the two second-epoch detections
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Considering the candidate 191092_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191092_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 191121_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191121_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 191122_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191122_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 191132_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191132_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 191140_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191140_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 191144_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191144_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
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Considering the candidate 191149_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191149_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 191151_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191151_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 191154_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191154_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 191158_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191158_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 191162_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191162_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (30.9") between the two second-epoch detections
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Considering the candidate 191164_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191164_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191171_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191171_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 191172_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191172_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 191178_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191178_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 191180_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191180_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 191183_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191183_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 191186_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191186_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 191187_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191187_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 191188_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191188_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191191_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191191_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 191192_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191192_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191194_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191194_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 191197_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191197_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191198_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191198_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (33.1") between the two second-epoch detections
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Considering the candidate 191204_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191204_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 191207_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191207_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 191210_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191210_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191213_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191213_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191214_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191214_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191216_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191216_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 191218_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191218_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191219_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191219_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 191224_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191224_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191228_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191228_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 191229_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191229_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191232_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191232_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 191234_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191234_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 191237_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191237_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 191242_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191242_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 191243_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191243_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191244_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191244_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191245_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191245_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 191246_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191246_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 191249_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191249_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 191250_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191250_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 191251_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191251_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191254_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191254_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191256_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191256_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 191259_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191259_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191260_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191260_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (32.3") between the two second-epoch detections
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Considering the candidate 191261_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191261_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191262_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191262_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 191263_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191263_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 191264_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191264_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 191267_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191267_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 191269_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191269_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 191270_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191270_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191273_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191273_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191277_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191277_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 191278_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191278_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 191282_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191282_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 191286_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191286_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191287_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191287_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 191289_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191289_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (39.8") between the two second-epoch detections
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Considering the candidate 191290_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191290_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191291_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191291_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 191299_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191299_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 191300_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191300_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191309_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191309_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 191311_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191311_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 191316_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191316_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 191318_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191318_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191322_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191322_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 191327_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191327_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 191329_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191329_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191330_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191330_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191331_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191331_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 191332_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191332_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191333_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191333_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 191336_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191336_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191343_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191343_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191346_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191346_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191347_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191347_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191351_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191351_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 191354_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191354_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191357_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191357_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191358_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191358_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 191361_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191361_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 191363_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191363_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 191366_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191366_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 191370_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191370_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 191374_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191374_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 191378_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191378_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 191381_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191381_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191382_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191382_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191384_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191384_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191386_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191386_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191387_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191387_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 191388_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191388_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191398_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191398_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 191401_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191401_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191402_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191402_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 191403_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191403_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 191408_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191408_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 191411_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191411_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 191414_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191414_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 191416_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191416_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (30.8") between the two second-epoch detections
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Considering the candidate 191418_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191418_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 191420_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191420_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191422_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191422_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 191426_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191426_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 191427_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191427_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191433_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191433_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 191434_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191434_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191436_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191436_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191438_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191438_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191439_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191439_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 191441_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191441_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191450_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191450_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 191451_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191451_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 191452_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191452_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 191455_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191455_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 191456_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191456_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191457_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191457_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 191459_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191459_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 191462_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191462_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 191463_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191463_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191468_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191468_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 191474_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191474_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 191478_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191478_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191480_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191480_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 191481_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191481_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191482_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191482_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 191483_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191483_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 191485_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191485_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 191486_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191486_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191489_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191489_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191491_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191491_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 191493_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191493_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191498_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191498_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 191500_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191500_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 191501_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191501_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
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Considering the candidate 191502_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191502_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191504_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191504_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191507_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191507_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 191508_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191508_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 191509_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191509_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (30.0") between the two second-epoch detections
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Considering the candidate 191510_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191510_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191511_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191511_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191512_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191512_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 191515_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191515_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 191517_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191517_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191519_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191519_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (44.2") between the two second-epoch detections
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Considering the candidate 191524_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191524_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191526_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191526_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 191529_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191529_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191530_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191530_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 191533_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191533_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 191534_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191534_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191537_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191537_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191538_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191538_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191539_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191539_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191540_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191540_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 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 191542_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191542_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 191544_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191544_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 191552_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191552_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 191555_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191555_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 191559_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191559_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 191560_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191560_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 191561_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191561_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 191563_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191563_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191566_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191566_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 191567_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191567_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 191568_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191568_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 191570_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191570_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191572_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191572_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 191573_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191573_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 191576_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191576_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191578_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191578_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191580_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191580_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 191581_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191581_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 191583_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191583_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191584_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191584_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 191585_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191585_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 191587_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191587_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
**** FOUND 00:24:56.08 +57:05:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191590_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191590_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191592_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191592_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191593_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191593_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191594_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191594_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 191597_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191597_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 191598_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191598_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 191599_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191599_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191603_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191603_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191608_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191608_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191609_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191609_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191615_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191615_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191616_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191616_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 191618_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191618_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 191623_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191623_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191624_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191624_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191625_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191625_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 191628_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191628_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 191629_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191629_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 191630_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191630_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191631_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191631_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 191641_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191641_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 191642_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191642_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191643_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191643_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 191644_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191644_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191645_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191645_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 191648_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191648_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 191652_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191652_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191660_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191660_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 191661_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191661_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191662_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191662_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 191664_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191664_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 191665_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191665_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 191666_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191666_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 191670_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191670_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191675_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191675_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191677_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191677_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191680_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191680_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 191683_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191683_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 191684_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191684_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191686_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191686_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 191687_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191687_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191689_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191689_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
**** FOUND 00:30:23.79 +55:49:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191692_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191692_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 191693_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191693_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 191695_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191695_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
**** FOUND 00:31:10.10 +55:39:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191699_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191699_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191701_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191701_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191706_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191706_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191710_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191710_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 191711_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191711_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 191713_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191713_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 191714_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191714_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 191718_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191718_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191719_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191719_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191769_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191769_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 191799_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191799_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 191812_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191812_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 191813_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191813_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
**** FOUND 00:28:42.42 +57:00:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191832_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191832_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191865_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191865_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191867_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191867_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191873_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191873_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 191894_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191894_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 191915_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191915_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 191938_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191938_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191954_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191954_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 191972_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191972_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191975_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191975_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 191977_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191977_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 191983_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191983_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 191985_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 191985_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 191994_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191994_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 191995_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 191995_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 192004_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192004_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192005_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192005_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 192009_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192009_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 192016_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192016_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (30.3") between the two second-epoch detections
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Considering the candidate 192019_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192019_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 192027_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192027_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 192052_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192052_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192057_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192057_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192062_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192062_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 192079_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192079_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192088_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192088_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192100_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192100_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 192106_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192106_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192111_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192111_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 192116_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192116_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 192117_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192117_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192124_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192124_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 192133_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192133_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192140_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192140_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192147_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192147_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 192154_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192154_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192155_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192155_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192160_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192160_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 192168_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192168_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 192176_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192176_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 192180_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192180_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192186_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192186_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192192_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192192_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192194_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192194_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192196_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192196_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192200_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192200_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 192206_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192206_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192211_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192211_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192218_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192218_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192219_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192219_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192221_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192221_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192241_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192241_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 192252_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192252_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 192253_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192253_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192254_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192254_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192257_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192257_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192261_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192261_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192262_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192262_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192294_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192294_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192295_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192295_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 192297_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192297_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 192301_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192301_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 192310_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192310_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 192314_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192314_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192317_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192317_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 192322_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192322_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192323_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192323_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192332_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192332_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192334_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192334_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192336_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192336_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 192338_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192338_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 192342_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192342_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192343_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192343_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 192346_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192346_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192355_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192355_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192356_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192356_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192357_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192357_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192361_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192361_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192367_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192367_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 192369_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192369_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 192376_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192376_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192379_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192379_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 192380_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192380_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 192382_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192382_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192383_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192383_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 192384_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192384_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 192393_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192393_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192394_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192394_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 192402_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192402_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192408_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192408_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192409_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192409_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192415_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192415_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 192416_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192416_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 192420_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192420_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 192423_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192423_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192427_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192427_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 192430_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192430_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 192432_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192432_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 192434_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192434_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 192441_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192441_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192442_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192442_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192450_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192450_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 192452_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192452_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 192453_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192453_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 192456_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192456_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 192458_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192458_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192461_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192461_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 192463_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192463_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192465_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192465_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192468_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192468_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 192469_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192469_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192472_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192472_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 192475_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192475_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 192476_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192476_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192477_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192477_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192478_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192478_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192479_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192479_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192483_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192483_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 192484_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192484_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
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Considering the candidate 192486_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192486_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 192498_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192498_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192500_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192500_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192504_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192504_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 192507_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192507_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
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Considering the candidate 192508_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192508_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192510_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192510_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 192516_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192516_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192534_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192534_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 192535_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192535_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192537_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192537_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (29.3") between the two second-epoch detections
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Considering the candidate 192539_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192539_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.1") between the two second-epoch detections
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Considering the candidate 192541_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192541_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192543_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192543_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192544_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192544_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 192549_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192549_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192551_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192551_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192553_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192553_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 192558_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192558_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 192561_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192561_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 192562_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192562_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 192570_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192570_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (32.1") between the two second-epoch detections
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Considering the candidate 192574_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192574_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 192579_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192579_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192580_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192580_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 192582_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192582_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192583_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192583_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 192584_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192584_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 192585_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192585_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192586_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192586_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192587_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192587_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192588_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192588_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 192592_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192592_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 192595_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192595_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192596_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192596_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192597_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192597_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192600_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192600_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 192602_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192602_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192604_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192604_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 192611_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192611_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 192612_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192612_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 192614_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192614_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192615_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192615_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192616_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192616_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 192619_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192619_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192621_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192621_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192622_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192622_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192623_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192623_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192631_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192631_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 192634_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192634_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192637_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192637_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192639_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192639_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192640_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192640_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192641_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192641_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192643_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192643_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192645_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192645_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 192647_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192647_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 192652_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192652_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192653_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192653_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 192656_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192656_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192657_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192657_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192658_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192658_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192672_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192672_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 192674_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192674_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 192677_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192677_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192678_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192678_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192679_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192679_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192681_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192681_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192683_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192683_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192686_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192686_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192689_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192689_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 192691_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192691_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 192694_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192694_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 192696_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192696_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192698_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192698_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192699_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192699_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192700_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192700_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192703_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192703_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192705_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192705_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 192707_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192707_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192712_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192712_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192715_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192715_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 192717_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192717_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 192720_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192720_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192721_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192721_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (51.0") between the two second-epoch detections
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Considering the candidate 192722_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192722_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192723_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192723_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 192727_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192727_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192728_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192728_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192731_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192731_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192734_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192734_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 192738_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192738_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192739_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192739_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192741_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192741_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 192744_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192744_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192745_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192745_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 192746_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192746_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192747_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192747_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 192750_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192750_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 192756_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192756_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 192761_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192761_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 192762_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192762_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 192763_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192763_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
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Considering the candidate 192765_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192765_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 192766_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192766_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192767_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192767_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192771_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192771_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 192773_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192773_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192774_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192774_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192776_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192776_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192777_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192777_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 192778_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192778_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192780_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192780_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 192781_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192781_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 192785_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192785_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192791_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192791_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 192793_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192793_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192794_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192794_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192795_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192795_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192797_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192797_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192799_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192799_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 192803_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192803_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 192807_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192807_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 192809_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192809_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192811_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192811_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 192817_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192817_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 192819_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192819_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192821_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192821_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192826_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192826_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 192828_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192828_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192829_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192829_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 192834_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192834_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 192835_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192835_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192836_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192836_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192840_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192840_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 192842_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192842_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 192846_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192846_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 192847_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192847_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 192850_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192850_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 192851_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192851_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 192852_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192852_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192854_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192854_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192855_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192855_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192857_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192857_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192859_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192859_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 192860_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192860_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192864_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192864_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192866_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192866_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192867_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192867_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 192870_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192870_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192873_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192873_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 192874_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192874_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192877_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192877_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 192881_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192881_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
**** FOUND 00:24:15.51 +52:02:07.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192885_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192885_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192887_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192887_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192888_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192888_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192890_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192890_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 192893_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192893_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192894_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192894_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192895_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192895_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192898_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192898_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192899_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192899_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192900_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192900_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192904_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192904_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192905_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192905_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192906_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192906_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 192907_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192907_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192908_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192908_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 192910_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192910_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 192911_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192911_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192914_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192914_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192922_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192922_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192924_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192924_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192925_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192925_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192928_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192928_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 192929_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192929_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 192932_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192932_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192934_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192934_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192937_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192937_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 192941_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192941_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 192943_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192943_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192945_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192945_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192946_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192946_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (34.7") between the two second-epoch detections
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Considering the candidate 192947_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192947_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192949_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192949_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 192950_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192950_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 192951_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192951_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 192952_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192952_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 192953_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192953_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192954_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192954_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 192955_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192955_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192957_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192957_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 192960_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192960_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 192961_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192961_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 192962_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192962_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 192963_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192963_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 192964_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192964_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192965_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192965_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 192971_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192971_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 192972_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192972_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 192977_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192977_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 192979_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192979_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 192982_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192982_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 192984_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192984_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 192985_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192985_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 192986_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192986_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192987_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192987_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 192988_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192988_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 192989_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192989_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192994_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192994_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192995_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192995_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 192996_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192996_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192997_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192997_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192998_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 192998_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 192999_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 192999_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193000_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193000_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193002_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193002_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 193004_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193004_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 193005_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193005_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (34.6") between the two second-epoch detections
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Considering the candidate 193011_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193011_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 193012_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193012_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193013_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193013_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193015_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193015_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193019_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193019_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193020_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193020_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193022_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193022_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193023_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193023_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 193024_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193024_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 193025_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193025_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193027_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193027_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 193028_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193028_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193032_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193032_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193034_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193034_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 193035_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193035_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 193039_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193039_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193040_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193040_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193041_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193041_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 193046_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193046_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 193049_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193049_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193050_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193050_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 193052_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193052_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 193053_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193053_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 193055_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193055_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 193056_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193056_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193057_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193057_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 193058_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193058_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193061_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193061_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 193062_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193062_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193064_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193064_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193069_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193069_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193070_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193070_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 193072_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193072_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193073_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193073_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193074_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193074_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 193075_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193075_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 193079_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193079_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193080_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193080_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 193083_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193083_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193086_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193086_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 193090_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193090_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193091_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193091_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193094_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193094_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193097_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193097_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 193099_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193099_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 193101_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193101_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193102_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193102_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193103_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193103_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 193104_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193104_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193107_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193107_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 193110_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193110_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193111_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193111_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 193115_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193115_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193128_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193128_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193129_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193129_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 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 193133_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193133_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193136_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193136_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
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Considering the candidate 193139_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193139_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193141_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193141_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193144_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193144_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 193152_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193152_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193153_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193153_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 193154_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193154_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 193156_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193156_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 193157_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193157_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193159_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193159_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 193160_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193160_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 193161_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193161_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193163_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193163_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193165_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193165_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 193166_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193166_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193170_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193170_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 193172_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193172_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 193178_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193178_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193180_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193180_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 193186_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193186_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 193192_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193192_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 193193_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193193_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 193208_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193208_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193216_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193216_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193222_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193222_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193223_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193223_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 193226_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193226_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 193236_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193236_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (24.1") between the two second-epoch detections
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Considering the candidate 193238_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193238_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 193240_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193240_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193242_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193242_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193245_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193245_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 193252_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193252_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 193255_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193255_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 193257_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193257_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 193260_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193260_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 193263_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193263_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 193264_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193264_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 193272_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193272_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 193284_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193284_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 193287_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193287_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193288_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193288_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193293_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193293_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193296_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193296_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193301_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193301_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193307_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193307_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 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 193313_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193313_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193314_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193314_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 193315_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193315_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193317_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193317_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 193319_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193319_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 193321_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193321_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 193326_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193326_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 193328_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193328_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 193331_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193331_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 193332_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193332_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 193338_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193338_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 193339_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193339_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 193345_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193345_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 193354_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193354_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 193357_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193357_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 193367_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193367_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193368_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193368_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 193373_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193373_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 193376_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193376_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 193377_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193377_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 193379_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193379_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193389_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193389_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (33.2") between the two second-epoch detections
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Considering the candidate 193393_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193393_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 193394_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193394_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193398_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193398_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 193403_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193403_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193411_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193411_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193427_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193427_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 193437_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193437_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 193439_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193439_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 193450_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193450_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 193456_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193456_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 193457_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193457_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 193459_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193459_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 193494_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193494_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 193501_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193501_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
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Considering the candidate 193505_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193505_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 193513_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193513_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 193515_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193515_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 193522_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193522_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 193530_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193530_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 193531_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193531_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 193536_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193536_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 193543_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193543_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 193546_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193546_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193567_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193567_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 193586_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193586_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 193621_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193621_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 193625_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193625_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 193628_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193628_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 193633_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193633_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 193643_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193643_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 193645_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193645_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 193646_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193646_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 193647_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193647_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 193650_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193650_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 193656_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193656_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (33.7") between the two second-epoch detections
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Considering the candidate 193744_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193744_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 193755_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193755_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 193767_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193767_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 193775_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193775_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 193789_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193789_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193812_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193812_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 193834_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193834_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 193861_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193861_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 193877_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193877_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (34.4") between the two second-epoch detections
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Considering the candidate 193896_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193896_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 193920_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193920_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 193982_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 193982_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 193987_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 193987_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 194011_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194011_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 194028_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194028_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 194036_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194036_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 194048_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194048_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 194106_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194106_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 194117_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194117_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 194133_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194133_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 194211_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194211_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 194279_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194279_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (57.9") between the two second-epoch detections
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Considering the candidate 194342_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194342_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194348_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194348_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (33.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194370_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 194370_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194625_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 194625_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
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Considering the candidate 140320_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 140320_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
**** FOUND 23:44:32.05 +56:34:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139426_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 139426_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35911_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
The candidate 35911_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75760_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
Preparing report for the candidate 75760_fd_Cas-04-Q2b1x1_2026-07-13_01-55-38_20.00sec_5.00C_LIGHT_0077
make_report_in_HTML.sh Phase 2 (HTML assembly): 15s
make_report_in_HTML.sh TOTAL: 687s
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 ####
00:09:29.89 +51:35:56.4
23:11:50.17 +56:02:36.5
00:23:39.91 +53:29:32.0
23:46:41.61 +54:28:42.6
00:23:06.20 +51:46:47.4
23:31:49.50 +55:35:28.2
23:46:35.12 +54:28:36.8
00:19:58.34 +51:55:30.9
23:36:38.52 +51:42:55.0
23:25:20.30 +56:49:19.5
23:57:30.50 +54:23:42.9
23:21:45.74 +54:26:17.6
23:16:38.24 +57:25:37.4
23:13:08.93 +56:57:55.6
23:11:50.98 +56:02:39.9
00:25:08.99 +56:12:31.0
00:23:37.31 +55:20:26.7
00:31:20.89 +57:06:28.4
00:16:33.45 +54:59:15.9
00:25:48.45 +51:44:26.3
00:19:52.20 +52:16:55.0
00:18:36.10 +56:44:54.8
00:23:50.32 +50:48:29.0
00:26:53.21 +56:55:11.3
00:25:28.39 +53:44:31.2
00:25:08.57 +56:25:14.8
00:26:39.90 +55:47:37.7
00:29:45.46 +55:26:25.4
00:19:11.65 +50:41:05.8
00:16:19.05 +53:07:30.1
00:28:49.63 +53:12:01.3
00:21:00.51 +52:22:38.5
00:21:16.93 +52:15:27.7
00:11:21.70 +52:13:52.0
00:23:42.53 +53:02:06.5
00:19:34.70 +53:55:07.7
00:21:10.51 +54:55:18.0
00:31:04.51 +55:56:03.4
00:30:00.23 +57:34:37.8
00:22:26.27 +50:18:54.7
00:13:44.77 +51:40:32.5
00:20:24.11 +51:48:24.3
00:11:07.36 +54:58:20.1
00:23:25.61 +50:26:02.3
00:02:21.53 +52:42:49.5
00:16:40.06 +52:14:35.6
00:18:01.69 +50:32:50.2
00:24:27.31 +57:21:46.5
23:49:33.87 +55:08:18.7
00:27:06.63 +50:36:29.3
00:05:25.34 +56:43:01.1
00:07:15.80 +50:53:28.8
00:20:47.25 +53:49:55.8
23:52:10.53 +50:21:19.9
00:15:11.91 +53:08:55.7
00:14:26.81 +50:19:37.6
00:15:46.28 +52:31:20.1
00:04:31.58 +52:54:29.4
00:17:56.73 +54:53:04.5
00:06:34.62 +54:54:42.1
23:57:47.87 +56:36:56.2
00:17:42.72 +53:39:39.1
00:21:54.66 +54:13:19.1
00:23:47.89 +51:26:19.6
00:26:32.41 +53:23:37.5
00:07:36.26 +55:01:28.7
23:16:59.96 +56:24:23.4
00:25:01.16 +55:19:54.8
00:26:03.61 +57:31:00.9
00:26:29.58 +57:34:31.3
00:08:41.39 +53:05:02.5
00:21:16.64 +54:40:28.1
00:19:51.47 +49:58:31.6
23:57:46.81 +52:11:11.3
00:29:02.41 +55:22:39.7
00:19:44.46 +51:33:12.2
00:17:35.04 +53:03:34.7
00:20:43.80 +54:00:53.8
23:57:09.66 +50:28:26.1
00:13:39.50 +56:53:46.2
00:25:19.81 +55:26:51.3
00:19:32.75 +57:40:55.6
00:31:44.06 +56:11:45.7
00:17:26.62 +49:47:25.8
00:07:57.56 +52:30:05.1
23:52:40.10 +50:22:49.0
00:26:25.79 +51:06:49.6
23:33:26.19 +50:19:13.1
00:27:57.22 +51:38:49.2
00:09:05.15 +53:32:52.1
00:24:17.17 +51:18:55.2
00:30:06.96 +55:40:15.5
00:18:22.11 +56:40:04.9
00:30:59.57 +57:25:04.4
00:27:16.60 +50:21:07.3
00:26:50.34 +50:01:56.9
00:23:52.33 +53:12:05.9
00:24:32.66 +50:12:45.2
00:05:35.28 +53:09:22.8
00:28:36.83 +57:13:19.5
00:25:21.82 +52:37:58.0
00:31:11.03 +55:35:42.6
00:30:02.61 +57:31:36.2
00:25:27.09 +50:00:26.5
00:28:32.21 +51:40:59.2
00:30:26.43 +55:57:29.1
00:28:43.64 +53:35:06.8
00:31:11.54 +56:01:45.2
00:28:15.30 +52:44:18.1
00:30:30.72 +55:12:22.2
00:17:29.39 +52:44:47.7
00:19:26.56 +54:51:21.8
00:31:08.08 +57:01:57.2
00:24:55.10 +50:43:56.9
00:31:58.07 +57:30:55.6
00:16:18.03 +55:02:57.1
00:24:33.64 +50:28:22.8
00:24:19.22 +49:57:03.6
00:24:27.91 +57:11:49.9
00:32:02.90 +57:43:25.8
23:32:13.83 +53:34:05.7
00:10:15.52 +53:28:38.1
00:16:09.79 +50:03:00.1
00:25:19.19 +57:25:08.3
00:13:35.35 +52:46:38.3
00:25:30.01 +49:43:57.0
00:27:39.18 +50:22:51.4
00:22:01.91 +51:22:31.0
00:28:04.73 +57:36:04.4
00:22:40.91 +50:29:36.0
00:26:30.66 +57:24:44.4
00:15:38.78 +53:48:04.1
00:26:09.86 +50:22:56.2
00:25:53.58 +53:52:55.2
00:24:54.84 +54:39:08.3
00:25:29.74 +55:20:20.4
00:24:26.76 +55:37:43.0
00:17:58.75 +53:30:39.8
00:21:18.69 +51:09:17.7
00:28:36.32 +52:45:09.1
00:18:39.72 +50:29:11.2
00:26:48.99 +50:20:31.3
00:18:09.60 +50:01:26.6
00:10:39.55 +50:02:31.4
00:19:08.44 +52:18:48.1
00:18:11.77 +53:11:42.1
00:26:38.20 +51:44:56.0
00:23:32.61 +55:48:00.5
00:27:57.97 +51:44:12.5
00:23:54.91 +50:22:50.0
00:27:16.82 +49:54:40.3
00:25:25.68 +49:53:23.2
00:24:26.36 +53:32:29.6
00:25:48.36 +53:57:27.4
00:22:25.25 +51:23:55.3
00:20:50.70 +50:44:15.7
00:25:34.05 +51:58:55.4
00:19:43.91 +51:43:50.6
00:24:23.63 +50:19:40.3
00:28:27.49 +52:13:56.6
00:25:02.99 +53:23:18.1
00:27:19.19 +57:11:04.1
00:18:15.79 +49:56:31.0
00:24:29.14 +53:23:18.7
00:25:28.88 +50:20:21.6
00:22:29.93 +51:14:18.7
00:27:53.14 +51:36:40.1
00:25:40.54 +49:43:18.4
00:27:06.84 +53:36:16.6
00:25:59.87 +50:55:09.0
00:18:39.34 +50:08:44.0
00:25:00.01 +56:14:23.1
00:27:18.50 +51:50:42.3
00:27:32.04 +49:53:18.8
00:29:52.44 +53:42:26.9
00:26:06.36 +49:46:55.2
00:12:49.81 +56:38:44.7
00:20:54.83 +52:26:46.7
00:28:05.07 +52:23:38.9
00:12:11.56 +50:01:07.2
00:24:09.96 +50:15:32.5
00:26:27.67 +52:48:18.2
00:19:47.94 +49:56:35.6
00:26:28.07 +52:02:02.1
00:28:26.64 +52:38:28.9
00:27:12.85 +50:07:02.8
00:20:27.48 +52:05:03.1
00:28:22.86 +57:29:15.3
00:17:23.60 +51:25:21.8
00:26:07.92 +49:44:43.2
00:15:59.44 +49:51:23.2
00:27:39.88 +50:01:01.5
00:28:44.79 +55:16:06.5
23:54:55.73 +56:31:16.7
00:12:35.21 +52:01:41.7
00:27:47.97 +52:08:25.3
00:25:14.90 +49:51:28.7
00:20:08.60 +53:27:53.1
00:30:07.09 +56:57:05.6
00:19:42.19 +52:22:46.0
00:26:51.01 +49:46:16.4
00:21:27.38 +50:49:24.9
00:22:10.45 +52:54:58.0
00:22:17.09 +52:50:24.0
00:26:21.17 +50:40:28.0
00:26:48.60 +52:36:36.7
00:29:07.59 +52:19:12.8
00:21:08.05 +51:41:04.5
00:24:02.78 +55:28:19.1
00:26:00.38 +51:13:40.9
00:27:11.52 +51:41:47.4
00:27:12.40 +54:18:54.6
00:24:24.90 +52:58:26.1
00:19:04.80 +51:18:58.4
00:18:44.49 +51:17:52.0
00:28:50.00 +52:17:32.3
00:25:12.60 +56:31:45.4
00:15:49.15 +50:44:30.1
00:17:13.10 +57:50:20.7
00:26:45.25 +51:29:25.7
00:27:23.78 +54:00:55.1
23:23:39.95 +49:26:42.9
00:25:18.10 +57:04:42.7
00:17:18.60 +57:02:33.1
00:27:57.87 +53:27:54.7
00:26:35.77 +52:23:53.9
00:16:16.13 +56:02:21.4
00:30:18.77 +56:07:42.4
00:28:36.78 +57:23:02.9
00:15:55.99 +51:39:55.6
00:24:40.29 +55:59:40.1
00:30:54.29 +55:16:20.2
00:10:32.47 +52:19:31.2
00:13:38.27 +54:57:36.2
00:21:43.15 +54:48:13.6
00:16:25.43 +53:02:33.7
00:30:41.22 +55:28:16.4
23:55:17.80 +56:36:24.9
00:29:26.67 +55:24:39.1
00:19:51.26 +57:01:50.4
23:57:06.71 +51:17:45.6
00:10:31.73 +53:26:21.2
00:12:02.75 +54:10:32.6
00:07:57.79 +53:09:53.4
00:17:14.21 +56:19:32.5
00:24:47.09 +56:08:45.9
00:30:39.20 +57:46:18.9
23:29:35.40 +53:27:37.2
23:45:36.35 +50:06:48.3
23:32:07.61 +51:53:29.5
23:41:05.57 +55:10:25.8
23:23:00.98 +49:26:22.2
23:16:55.27 +56:25:16.9
00:25:59.25 +53:55:33.9
########### 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 ####
23:11:50.17 +56:02:36.5
00:23:39.91 +53:29:32.0
23:46:41.61 +54:28:42.6
00:23:06.20 +51:46:47.4
23:31:49.50 +55:35:28.2
23:46:35.12 +54:28:36.8
00:19:58.34 +51:55:30.9
23:36:38.52 +51:42:55.0
23:25:20.30 +56:49:19.5
23:57:30.50 +54:23:42.9
23:21:45.74 +54:26:17.6
23:16:38.24 +57:25:37.4
23:13:08.93 +56:57:55.6
00:09:29.89 +51:35:56.4
00:25:08.99 +56:12:31.0
00:23:37.31 +55:20:26.7
00:31:20.89 +57:06:28.4
00:16:33.45 +54:59:15.9
00:25:48.45 +51:44:26.3
00:19:52.20 +52:16:55.0
00:18:36.10 +56:44:54.8
00:23:50.32 +50:48:29.0
00:26:53.21 +56:55:11.3
00:25:28.39 +53:44:31.2
00:25:08.57 +56:25:14.8
00:26:39.90 +55:47:37.7
00:29:45.46 +55:26:25.4
00:19:11.65 +50:41:05.8
00:16:19.05 +53:07:30.1
00:28:49.63 +53:12:01.3
00:21:00.51 +52:22:38.5
00:21:16.93 +52:15:27.7
00:11:21.70 +52:13:52.0
00:23:42.53 +53:02:06.5
00:19:34.70 +53:55:07.7
00:21:10.51 +54:55:18.0
00:31:04.51 +55:56:03.4
00:30:00.23 +57:34:37.8
00:22:26.27 +50:18:54.7
00:13:44.77 +51:40:32.5
00:20:24.11 +51:48:24.3
00:11:07.36 +54:58:20.1
00:23:25.61 +50:26:02.3
00:02:21.53 +52:42:49.5
00:16:40.06 +52:14:35.6
00:18:01.69 +50:32:50.2
00:24:27.31 +57:21:46.5
23:49:33.87 +55:08:18.7
00:27:06.63 +50:36:29.3
00:05:25.34 +56:43:01.1
00:07:15.80 +50:53:28.8
00:20:47.25 +53:49:55.8
23:52:10.53 +50:21:19.9
00:15:11.91 +53:08:55.7
00:14:26.81 +50:19:37.6
00:15:46.28 +52:31:20.1
00:04:31.58 +52:54:29.4
00:17:56.73 +54:53:04.5
00:06:34.62 +54:54:42.1
23:57:47.87 +56:36:56.2
00:17:42.72 +53:39:39.1
00:21:54.66 +54:13:19.1
00:23:47.89 +51:26:19.6
00:26:32.41 +53:23:37.5
00:07:36.26 +55:01:28.7
23:16:59.96 +56:24:23.4
00:25:01.16 +55:19:54.8
00:26:03.61 +57:31:00.9
00:26:29.58 +57:34:31.3
00:08:41.39 +53:05:02.5
00:21:16.64 +54:40:28.1
00:19:51.47 +49:58:31.6
23:57:46.81 +52:11:11.3
00:29:02.41 +55:22:39.7
00:19:44.46 +51:33:12.2
00:17:35.04 +53:03:34.7
00:20:43.80 +54:00:53.8
23:57:09.66 +50:28:26.1
00:13:39.50 +56:53:46.2
00:25:19.81 +55:26:51.3
00:19:32.75 +57:40:55.6
00:31:44.06 +56:11:45.7
00:17:26.62 +49:47:25.8
00:07:57.56 +52:30:05.1
23:52:40.10 +50:22:49.0
00:26:25.79 +51:06:49.6
23:33:26.19 +50:19:13.1
00:27:57.22 +51:38:49.2
00:09:05.15 +53:32:52.1
00:24:17.17 +51:18:55.2
00:30:06.96 +55:40:15.5
00:18:22.11 +56:40:04.9
00:30:59.57 +57:25:04.4
00:27:16.60 +50:21:07.3
00:26:50.34 +50:01:56.9
00:23:52.33 +53:12:05.9
00:24:32.66 +50:12:45.2
00:05:35.28 +53:09:22.8
00:28:36.83 +57:13:19.5
00:25:21.82 +52:37:58.0
00:31:11.03 +55:35:42.6
00:30:02.61 +57:31:36.2
00:25:27.09 +50:00:26.5
00:28:32.21 +51:40:59.2
00:30:26.43 +55:57:29.1
00:28:43.64 +53:35:06.8
00:31:11.54 +56:01:45.2
00:28:15.30 +52:44:18.1
00:30:30.72 +55:12:22.2
00:17:29.39 +52:44:47.7
00:19:26.56 +54:51:21.8
00:31:08.08 +57:01:57.2
00:24:55.10 +50:43:56.9
00:31:58.07 +57:30:55.6
00:16:18.03 +55:02:57.1
00:24:33.64 +50:28:22.8
00:24:19.22 +49:57:03.6
00:24:27.91 +57:11:49.9
00:32:02.90 +57:43:25.8
23:32:13.83 +53:34:05.7
00:10:15.52 +53:28:38.1
00:16:09.79 +50:03:00.1
00:25:19.19 +57:25:08.3
00:13:35.35 +52:46:38.3
00:25:30.01 +49:43:57.0
00:27:39.18 +50:22:51.4
00:22:01.91 +51:22:31.0
00:28:04.73 +57:36:04.4
00:22:40.91 +50:29:36.0
00:26:30.66 +57:24:44.4
00:15:38.78 +53:48:04.1
00:26:09.86 +50:22:56.2
00:25:53.58 +53:52:55.2
00:24:54.84 +54:39:08.3
00:25:29.74 +55:20:20.4
00:24:26.76 +55:37:43.0
00:17:58.75 +53:30:39.8
00:21:18.69 +51:09:17.7
00:28:36.32 +52:45:09.1
00:18:39.72 +50:29:11.2
00:26:48.99 +50:20:31.3
00:18:09.60 +50:01:26.6
00:10:39.55 +50:02:31.4
00:19:08.44 +52:18:48.1
00:18:11.77 +53:11:42.1
00:26:38.20 +51:44:56.0
00:23:32.61 +55:48:00.5
00:27:57.97 +51:44:12.5
00:23:54.91 +50:22:50.0
00:27:16.82 +49:54:40.3
00:25:25.68 +49:53:23.2
00:24:26.36 +53:32:29.6
00:25:48.36 +53:57:27.4
00:22:25.25 +51:23:55.3
00:20:50.70 +50:44:15.7
00:25:34.05 +51:58:55.4
00:19:43.91 +51:43:50.6
00:24:23.63 +50:19:40.3
00:28:27.49 +52:13:56.6
00:25:02.99 +53:23:18.1
00:27:19.19 +57:11:04.1
00:18:15.79 +49:56:31.0
00:24:29.14 +53:23:18.7
00:25:28.88 +50:20:21.6
00:22:29.93 +51:14:18.7
00:27:53.14 +51:36:40.1
00:25:40.54 +49:43:18.4
00:27:06.84 +53:36:16.6
00:25:59.87 +50:55:09.0
00:18:39.34 +50:08:44.0
00:25:00.01 +56:14:23.1
00:27:18.50 +51:50:42.3
00:27:32.04 +49:53:18.8
00:29:52.44 +53:42:26.9
00:26:06.36 +49:46:55.2
00:12:49.81 +56:38:44.7
00:20:54.83 +52:26:46.7
00:28:05.07 +52:23:38.9
00:12:11.56 +50:01:07.2
00:24:09.96 +50:15:32.5
00:26:27.67 +52:48:18.2
00:19:47.94 +49:56:35.6
00:26:28.07 +52:02:02.1
00:28:26.64 +52:38:28.9
00:27:12.85 +50:07:02.8
00:20:27.48 +52:05:03.1
00:28:22.86 +57:29:15.3
00:17:23.60 +51:25:21.8
00:26:07.92 +49:44:43.2
00:15:59.44 +49:51:23.2
00:27:39.88 +50:01:01.5
00:28:44.79 +55:16:06.5
23:54:55.73 +56:31:16.7
00:12:35.21 +52:01:41.7
00:27:47.97 +52:08:25.3
00:25:14.90 +49:51:28.7
00:20:08.60 +53:27:53.1
00:30:07.09 +56:57:05.6
00:19:42.19 +52:22:46.0
00:26:51.01 +49:46:16.4
00:21:27.38 +50:49:24.9
00:22:10.45 +52:54:58.0
00:22:17.09 +52:50:24.0
00:26:21.17 +50:40:28.0
00:26:48.60 +52:36:36.7
00:29:07.59 +52:19:12.8
00:21:08.05 +51:41:04.5
00:24:02.78 +55:28:19.1
00:26:00.38 +51:13:40.9
00:27:11.52 +51:41:47.4
00:27:12.40 +54:18:54.6
00:24:24.90 +52:58:26.1
00:19:04.80 +51:18:58.4
00:18:44.49 +51:17:52.0
00:28:50.00 +52:17:32.3
00:25:12.60 +56:31:45.4
00:15:49.15 +50:44:30.1
00:17:13.10 +57:50:20.7
00:26:45.25 +51:29:25.7
00:27:23.78 +54:00:55.1
23:23:39.95 +49:26:42.9
00:25:18.10 +57:04:42.7
00:17:18.60 +57:02:33.1
00:27:57.87 +53:27:54.7
00:26:35.77 +52:23:53.9
00:16:16.13 +56:02:21.4
00:30:18.77 +56:07:42.4
00:28:36.78 +57:23:02.9
00:15:55.99 +51:39:55.6
00:24:40.29 +55:59:40.1
00:30:54.29 +55:16:20.2
00:10:32.47 +52:19:31.2
00:13:38.27 +54:57:36.2
00:21:43.15 +54:48:13.6
00:16:25.43 +53:02:33.7
00:30:41.22 +55:28:16.4
23:55:17.80 +56:36:24.9
00:29:26.67 +55:24:39.1
00:19:51.26 +57:01:50.4
23:57:06.71 +51:17:45.6
00:10:31.73 +53:26:21.2
00:12:02.75 +54:10:32.6
00:07:57.79 +53:09:53.4
00:17:14.21 +56:19:32.5
00:24:47.09 +56:08:45.9
00:30:39.20 +57:46:18.9
23:29:35.40 +53:27:37.2
23:45:36.35 +50:06:48.3
23:32:07.61 +51:53:29.5
23:41:05.57 +55:10:25.8
23:23:00.98 +49:26:22.2
23:16:55.27 +56:25:16.9
23:11:50.98 +56:02:39.9
00:25:59.25 +53:55:33.9
###################################################################################
23:11:50.17 +56:02:36.5 -- not an asteroid (will add it to exclusion list)
00:23:39.91 +53:29:32.0 -- not an asteroid (will add it to exclusion list)
23:46:41.61 +54:28:42.6 -- not an asteroid (will add it to exclusion list)
00:23:06.20 +51:46:47.4 -- not an asteroid (will add it to exclusion list)
23:31:49.50 +55:35:28.2 -- not an asteroid (will add it to exclusion list)
23:46:35.12 +54:28:36.8 -- not an asteroid (will add it to exclusion list)
00:19:58.34 +51:55:30.9 -- not an asteroid (will add it to exclusion list)
23:36:38.52 +51:42:55.0 -- not an asteroid (will add it to exclusion list)
23:25:20.30 +56:49:19.5 -- not an asteroid (will add it to exclusion list)
23:57:30.50 +54:23:42.9 -- not an asteroid (will add it to exclusion list)
23:21:45.74 +54:26:17.6 -- not an asteroid (will add it to exclusion list)
23:16:38.24 +57:25:37.4 -- not an asteroid (will add it to exclusion list)
23:13:08.93 +56:57:55.6 -- not an asteroid (will add it to exclusion list)
00:09:29.89 +51:35:56.4 -- not an asteroid (will add it to exclusion list)
00:25:08.99 +56:12:31.0 -- not an asteroid (will add it to exclusion list)
00:23:37.31 +55:20:26.7 -- not an asteroid (will add it to exclusion list)
00:31:20.89 +57:06:28.4 -- not an asteroid (will add it to exclusion list)
00:16:33.45 +54:59:15.9 -- not an asteroid (will add it to exclusion list)
00:25:48.45 +51:44:26.3 -- not an asteroid (will add it to exclusion list)
00:19:52.20 +52:16:55.0 -- not an asteroid (will add it to exclusion list)
00:18:36.10 +56:44:54.8 -- not an asteroid (will add it to exclusion list)
00:23:50.32 +50:48:29.0 -- not an asteroid (will add it to exclusion list)
00:26:53.21 +56:55:11.3 -- not an asteroid (will add it to exclusion list)
00:25:28.39 +53:44:31.2 -- not an asteroid (will add it to exclusion list)
00:25:08.57 +56:25:14.8 -- not an asteroid (will add it to exclusion list)
00:26:39.90 +55:47:37.7 -- not an asteroid (will add it to exclusion list)
00:29:45.46 +55:26:25.4 -- not an asteroid (will add it to exclusion list)
00:19:11.65 +50:41:05.8 -- not an asteroid (will add it to exclusion list)
00:16:19.05 +53:07:30.1 -- not an asteroid (will add it to exclusion list)
00:28:49.63 +53:12:01.3 -- not an asteroid (will add it to exclusion list)
00:21:00.51 +52:22:38.5 -- not an asteroid (will add it to exclusion list)
00:21:16.93 +52:15:27.7 -- not an asteroid (will add it to exclusion list)
00:11:21.70 +52:13:52.0 -- not an asteroid (will add it to exclusion list)
00:23:42.53 +53:02:06.5 -- not an asteroid (will add it to exclusion list)
00:19:34.70 +53:55:07.7 -- not an asteroid (will add it to exclusion list)
00:21:10.51 +54:55:18.0 -- not an asteroid (will add it to exclusion list)
00:31:04.51 +55:56:03.4 -- not an asteroid (will add it to exclusion list)
00:30:00.23 +57:34:37.8 -- not an asteroid (will add it to exclusion list)
00:22:26.27 +50:18:54.7 -- not an asteroid (will add it to exclusion list)
00:13:44.77 +51:40:32.5 -- not an asteroid (will add it to exclusion list)
00:20:24.11 +51:48:24.3 -- not an asteroid (will add it to exclusion list)
00:11:07.36 +54:58:20.1 -- not an asteroid (will add it to exclusion list)
00:23:25.61 +50:26:02.3 -- not an asteroid (will add it to exclusion list)
00:02:21.53 +52:42:49.5 -- not an asteroid (will add it to exclusion list)
00:16:40.06 +52:14:35.6 -- not an asteroid (will add it to exclusion list)
00:18:01.69 +50:32:50.2 -- not an asteroid (will add it to exclusion list)
00:24:27.31 +57:21:46.5 -- not an asteroid (will add it to exclusion list)
23:49:33.87 +55:08:18.7 -- not an asteroid (will add it to exclusion list)
00:27:06.63 +50:36:29.3 -- not an asteroid (will add it to exclusion list)
00:05:25.34 +56:43:01.1 -- not an asteroid (will add it to exclusion list)
00:07:15.80 +50:53:28.8 -- not an asteroid (will add it to exclusion list)
00:20:47.25 +53:49:55.8 -- not an asteroid (will add it to exclusion list)
23:52:10.53 +50:21:19.9 -- not an asteroid (will add it to exclusion list)
00:15:11.91 +53:08:55.7 -- not an asteroid (will add it to exclusion list)
00:14:26.81 +50:19:37.6 -- not an asteroid (will add it to exclusion list)
00:15:46.28 +52:31:20.1 -- not an asteroid (will add it to exclusion list)
00:04:31.58 +52:54:29.4 -- not an asteroid (will add it to exclusion list)
00:17:56.73 +54:53:04.5 -- not an asteroid (will add it to exclusion list)
00:06:34.62 +54:54:42.1 -- not an asteroid (will add it to exclusion list)
23:57:47.87 +56:36:56.2 -- not an asteroid (will add it to exclusion list)
00:17:42.72 +53:39:39.1 -- not an asteroid (will add it to exclusion list)
00:21:54.66 +54:13:19.1 -- not an asteroid (will add it to exclusion list)
00:23:47.89 +51:26:19.6 -- not an asteroid (will add it to exclusion list)
00:26:32.41 +53:23:37.5 -- not an asteroid (will add it to exclusion list)
00:07:36.26 +55:01:28.7 -- not an asteroid (will add it to exclusion list)
23:16:59.96 +56:24:23.4 -- not an asteroid (will add it to exclusion list)
00:25:01.16 +55:19:54.8 -- not an asteroid (will add it to exclusion list)
00:26:03.61 +57:31:00.9 -- not an asteroid (will add it to exclusion list)
00:26:29.58 +57:34:31.3 -- not an asteroid (will add it to exclusion list)
00:08:41.39 +53:05:02.5 -- not an asteroid (will add it to exclusion list)
00:21:16.64 +54:40:28.1 -- not an asteroid (will add it to exclusion list)
00:19:51.47 +49:58:31.6 -- not an asteroid (will add it to exclusion list)
23:57:46.81 +52:11:11.3 -- not an asteroid (will add it to exclusion list)
00:29:02.41 +55:22:39.7 -- not an asteroid (will add it to exclusion list)
00:19:44.46 +51:33:12.2 -- not an asteroid (will add it to exclusion list)
00:17:35.04 +53:03:34.7 -- not an asteroid (will add it to exclusion list)
00:20:43.80 +54:00:53.8 -- not an asteroid (will add it to exclusion list)
23:57:09.66 +50:28:26.1 -- not an asteroid (will add it to exclusion list)
00:13:39.50 +56:53:46.2 -- not an asteroid (will add it to exclusion list)
00:25:19.81 +55:26:51.3 -- not an asteroid (will add it to exclusion list)
00:19:32.75 +57:40:55.6 -- not an asteroid (will add it to exclusion list)
00:31:44.06 +56:11:45.7 -- not an asteroid (will add it to exclusion list)
00:17:26.62 +49:47:25.8 -- not an asteroid (will add it to exclusion list)
00:07:57.56 +52:30:05.1 -- not an asteroid (will add it to exclusion list)
23:52:40.10 +50:22:49.0 -- not an asteroid (will add it to exclusion list)
00:26:25.79 +51:06:49.6 -- not an asteroid (will add it to exclusion list)
23:33:26.19 +50:19:13.1 -- not an asteroid (will add it to exclusion list)
00:27:57.22 +51:38:49.2 -- not an asteroid (will add it to exclusion list)
00:09:05.15 +53:32:52.1 -- not an asteroid (will add it to exclusion list)
00:24:17.17 +51:18:55.2 -- not an asteroid (will add it to exclusion list)
00:30:06.96 +55:40:15.5 -- not an asteroid (will add it to exclusion list)
00:18:22.11 +56:40:04.9 -- not an asteroid (will add it to exclusion list)
00:30:59.57 +57:25:04.4 -- not an asteroid (will add it to exclusion list)
00:27:16.60 +50:21:07.3 -- not an asteroid (will add it to exclusion list)
00:26:50.34 +50:01:56.9 -- not an asteroid (will add it to exclusion list)
00:23:52.33 +53:12:05.9 -- not an asteroid (will add it to exclusion list)
00:24:32.66 +50:12:45.2 -- not an asteroid (will add it to exclusion list)
00:05:35.28 +53:09:22.8 -- not an asteroid (will add it to exclusion list)
00:28:36.83 +57:13:19.5 -- not an asteroid (will add it to exclusion list)
00:25:21.82 +52:37:58.0 -- not an asteroid (will add it to exclusion list)
00:31:11.03 +55:35:42.6 -- not an asteroid (will add it to exclusion list)
00:30:02.61 +57:31:36.2 -- not an asteroid (will add it to exclusion list)
00:25:27.09 +50:00:26.5 -- not an asteroid (will add it to exclusion list)
00:28:32.21 +51:40:59.2 -- not an asteroid (will add it to exclusion list)
00:30:26.43 +55:57:29.1 -- not an asteroid (will add it to exclusion list)
00:28:43.64 +53:35:06.8 -- not an asteroid (will add it to exclusion list)
00:31:11.54 +56:01:45.2 -- not an asteroid (will add it to exclusion list)
00:28:15.30 +52:44:18.1 -- not an asteroid (will add it to exclusion list)
00:30:30.72 +55:12:22.2 -- not an asteroid (will add it to exclusion list)
00:17:29.39 +52:44:47.7 -- not an asteroid (will add it to exclusion list)
00:19:26.56 +54:51:21.8 -- not an asteroid (will add it to exclusion list)
00:31:08.08 +57:01:57.2 -- not an asteroid (will add it to exclusion list)
00:24:55.10 +50:43:56.9 -- not an asteroid (will add it to exclusion list)
00:31:58.07 +57:30:55.6 -- not an asteroid (will add it to exclusion list)
00:16:18.03 +55:02:57.1 -- not an asteroid (will add it to exclusion list)
00:24:33.64 +50:28:22.8 -- not an asteroid (will add it to exclusion list)
00:24:19.22 +49:57:03.6 -- not an asteroid (will add it to exclusion list)
00:24:27.91 +57:11:49.9 -- not an asteroid (will add it to exclusion list)
00:32:02.90 +57:43:25.8 -- not an asteroid (will add it to exclusion list)
23:32:13.83 +53:34:05.7 -- not an asteroid (will add it to exclusion list)
00:10:15.52 +53:28:38.1 -- not an asteroid (will add it to exclusion list)
00:16:09.79 +50:03:00.1 -- not an asteroid (will add it to exclusion list)
00:25:19.19 +57:25:08.3 -- not an asteroid (will add it to exclusion list)
00:13:35.35 +52:46:38.3 -- not an asteroid (will add it to exclusion list)
00:25:30.01 +49:43:57.0 -- not an asteroid (will add it to exclusion list)
00:27:39.18 +50:22:51.4 -- not an asteroid (will add it to exclusion list)
00:22:01.91 +51:22:31.0 -- not an asteroid (will add it to exclusion list)
00:28:04.73 +57:36:04.4 -- not an asteroid (will add it to exclusion list)
00:22:40.91 +50:29:36.0 -- not an asteroid (will add it to exclusion list)
00:26:30.66 +57:24:44.4 -- not an asteroid (will add it to exclusion list)
00:15:38.78 +53:48:04.1 -- not an asteroid (will add it to exclusion list)
00:26:09.86 +50:22:56.2 -- not an asteroid (will add it to exclusion list)
00:25:53.58 +53:52:55.2 -- not an asteroid (will add it to exclusion list)
00:24:54.84 +54:39:08.3 -- not an asteroid (will add it to exclusion list)
00:25:29.74 +55:20:20.4 -- not an asteroid (will add it to exclusion list)
00:24:26.76 +55:37:43.0 -- not an asteroid (will add it to exclusion list)
00:17:58.75 +53:30:39.8 -- not an asteroid (will add it to exclusion list)
00:21:18.69 +51:09:17.7 -- not an asteroid (will add it to exclusion list)
00:28:36.32 +52:45:09.1 -- not an asteroid (will add it to exclusion list)
00:18:39.72 +50:29:11.2 -- not an asteroid (will add it to exclusion list)
00:26:48.99 +50:20:31.3 -- not an asteroid (will add it to exclusion list)
00:18:09.60 +50:01:26.6 -- not an asteroid (will add it to exclusion list)
00:10:39.55 +50:02:31.4 -- not an asteroid (will add it to exclusion list)
00:19:08.44 +52:18:48.1 -- not an asteroid (will add it to exclusion list)
00:18:11.77 +53:11:42.1 -- not an asteroid (will add it to exclusion list)
00:26:38.20 +51:44:56.0 -- not an asteroid (will add it to exclusion list)
00:23:32.61 +55:48:00.5 -- not an asteroid (will add it to exclusion list)
00:27:57.97 +51:44:12.5 -- not an asteroid (will add it to exclusion list)
00:23:54.91 +50:22:50.0 -- not an asteroid (will add it to exclusion list)
00:27:16.82 +49:54:40.3 -- not an asteroid (will add it to exclusion list)
00:25:25.68 +49:53:23.2 -- not an asteroid (will add it to exclusion list)
00:24:26.36 +53:32:29.6 -- not an asteroid (will add it to exclusion list)
00:25:48.36 +53:57:27.4 -- not an asteroid (will add it to exclusion list)
00:22:25.25 +51:23:55.3 -- not an asteroid (will add it to exclusion list)
00:20:50.70 +50:44:15.7 -- not an asteroid (will add it to exclusion list)
00:25:34.05 +51:58:55.4 -- not an asteroid (will add it to exclusion list)
00:19:43.91 +51:43:50.6 -- not an asteroid (will add it to exclusion list)
00:24:23.63 +50:19:40.3 -- not an asteroid (will add it to exclusion list)
00:28:27.49 +52:13:56.6 -- not an asteroid (will add it to exclusion list)
00:25:02.99 +53:23:18.1 -- not an asteroid (will add it to exclusion list)
00:27:19.19 +57:11:04.1 -- not an asteroid (will add it to exclusion list)
00:18:15.79 +49:56:31.0 -- not an asteroid (will add it to exclusion list)
00:24:29.14 +53:23:18.7 -- not an asteroid (will add it to exclusion list)
00:25:28.88 +50:20:21.6 -- not an asteroid (will add it to exclusion list)
00:22:29.93 +51:14:18.7 -- not an asteroid (will add it to exclusion list)
00:27:53.14 +51:36:40.1 -- not an asteroid (will add it to exclusion list)
00:25:40.54 +49:43:18.4 -- not an asteroid (will add it to exclusion list)
00:27:06.84 +53:36:16.6 -- not an asteroid (will add it to exclusion list)
00:25:59.87 +50:55:09.0 -- not an asteroid (will add it to exclusion list)
00:18:39.34 +50:08:44.0 -- not an asteroid (will add it to exclusion list)
00:25:00.01 +56:14:23.1 -- not an asteroid (will add it to exclusion list)
00:27:18.50 +51:50:42.3 -- not an asteroid (will add it to exclusion list)
00:27:32.04 +49:53:18.8 -- not an asteroid (will add it to exclusion list)
00:29:52.44 +53:42:26.9 -- not an asteroid (will add it to exclusion list)
00:26:06.36 +49:46:55.2 -- not an asteroid (will add it to exclusion list)
00:12:49.81 +56:38:44.7 -- not an asteroid (will add it to exclusion list)
00:20:54.83 +52:26:46.7 -- not an asteroid (will add it to exclusion list)
00:28:05.07 +52:23:38.9 -- not an asteroid (will add it to exclusion list)
00:12:11.56 +50:01:07.2 -- not an asteroid (will add it to exclusion list)
00:24:09.96 +50:15:32.5 -- not an asteroid (will add it to exclusion list)
00:26:27.67 +52:48:18.2 -- not an asteroid (will add it to exclusion list)
00:19:47.94 +49:56:35.6 -- not an asteroid (will add it to exclusion list)
00:26:28.07 +52:02:02.1 -- not an asteroid (will add it to exclusion list)
00:28:26.64 +52:38:28.9 -- not an asteroid (will add it to exclusion list)
00:27:12.85 +50:07:02.8 -- not an asteroid (will add it to exclusion list)
00:20:27.48 +52:05:03.1 -- not an asteroid (will add it to exclusion list)
00:28:22.86 +57:29:15.3 -- not an asteroid (will add it to exclusion list)
00:17:23.60 +51:25:21.8 -- not an asteroid (will add it to exclusion list)
00:26:07.92 +49:44:43.2 -- not an asteroid (will add it to exclusion list)
00:15:59.44 +49:51:23.2 -- not an asteroid (will add it to exclusion list)
00:27:39.88 +50:01:01.5 -- not an asteroid (will add it to exclusion list)
00:28:44.79 +55:16:06.5 -- not an asteroid (will add it to exclusion list)
23:54:55.73 +56:31:16.7 -- not an asteroid (will add it to exclusion list)
00:12:35.21 +52:01:41.7 -- not an asteroid (will add it to exclusion list)
00:27:47.97 +52:08:25.3 -- not an asteroid (will add it to exclusion list)
00:25:14.90 +49:51:28.7 -- not an asteroid (will add it to exclusion list)
00:20:08.60 +53:27:53.1 -- not an asteroid (will add it to exclusion list)
00:30:07.09 +56:57:05.6 -- not an asteroid (will add it to exclusion list)
00:19:42.19 +52:22:46.0 -- not an asteroid (will add it to exclusion list)
00:26:51.01 +49:46:16.4 -- not an asteroid (will add it to exclusion list)
00:21:27.38 +50:49:24.9 -- not an asteroid (will add it to exclusion list)
00:22:10.45 +52:54:58.0 -- not an asteroid (will add it to exclusion list)
00:22:17.09 +52:50:24.0 -- not an asteroid (will add it to exclusion list)
00:26:21.17 +50:40:28.0 -- not an asteroid (will add it to exclusion list)
00:26:48.60 +52:36:36.7 -- not an asteroid (will add it to exclusion list)
00:29:07.59 +52:19:12.8 -- not an asteroid (will add it to exclusion list)
00:21:08.05 +51:41:04.5 -- not an asteroid (will add it to exclusion list)
00:24:02.78 +55:28:19.1 -- not an asteroid (will add it to exclusion list)
00:26:00.38 +51:13:40.9 -- not an asteroid (will add it to exclusion list)
00:27:11.52 +51:41:47.4 -- not an asteroid (will add it to exclusion list)
00:27:12.40 +54:18:54.6 -- not an asteroid (will add it to exclusion list)
00:24:24.90 +52:58:26.1 -- not an asteroid (will add it to exclusion list)
00:19:04.80 +51:18:58.4 -- not an asteroid (will add it to exclusion list)
00:18:44.49 +51:17:52.0 -- not an asteroid (will add it to exclusion list)
00:28:50.00 +52:17:32.3 -- not an asteroid (will add it to exclusion list)
00:25:12.60 +56:31:45.4 -- not an asteroid (will add it to exclusion list)
00:15:49.15 +50:44:30.1 -- not an asteroid (will add it to exclusion list)
00:17:13.10 +57:50:20.7 -- not an asteroid (will add it to exclusion list)
00:26:45.25 +51:29:25.7 -- not an asteroid (will add it to exclusion list)
00:27:23.78 +54:00:55.1 -- not an asteroid (will add it to exclusion list)
23:23:39.95 +49:26:42.9 -- not an asteroid (will add it to exclusion list)
00:25:18.10 +57:04:42.7 -- not an asteroid (will add it to exclusion list)
00:17:18.60 +57:02:33.1 -- not an asteroid (will add it to exclusion list)
00:27:57.87 +53:27:54.7 -- not an asteroid (will add it to exclusion list)
00:26:35.77 +52:23:53.9 -- not an asteroid (will add it to exclusion list)
00:16:16.13 +56:02:21.4 -- not an asteroid (will add it to exclusion list)
00:30:18.77 +56:07:42.4 -- not an asteroid (will add it to exclusion list)
00:28:36.78 +57:23:02.9 -- not an asteroid (will add it to exclusion list)
00:15:55.99 +51:39:55.6 -- not an asteroid (will add it to exclusion list)
00:24:40.29 +55:59:40.1 -- not an asteroid (will add it to exclusion list)
00:30:54.29 +55:16:20.2 -- not an asteroid (will add it to exclusion list)
00:10:32.47 +52:19:31.2 -- not an asteroid (will add it to exclusion list)
00:13:38.27 +54:57:36.2 -- not an asteroid (will add it to exclusion list)
00:21:43.15 +54:48:13.6 -- not an asteroid (will add it to exclusion list)
00:16:25.43 +53:02:33.7 -- not an asteroid (will add it to exclusion list)
00:30:41.22 +55:28:16.4 -- not an asteroid (will add it to exclusion list)
23:55:17.80 +56:36:24.9 -- not an asteroid (will add it to exclusion list)
00:29:26.67 +55:24:39.1 -- not an asteroid (will add it to exclusion list)
00:19:51.26 +57:01:50.4 -- not an asteroid (will add it to exclusion list)
23:57:06.71 +51:17:45.6 -- not an asteroid (will add it to exclusion list)
00:10:31.73 +53:26:21.2 -- not an asteroid (will add it to exclusion list)
00:12:02.75 +54:10:32.6 -- not an asteroid (will add it to exclusion list)
00:07:57.79 +53:09:53.4 -- not an asteroid (will add it to exclusion list)
00:17:14.21 +56:19:32.5 -- not an asteroid (will add it to exclusion list)
00:24:47.09 +56:08:45.9 -- not an asteroid (will add it to exclusion list)
00:30:39.20 +57:46:18.9 -- not an asteroid (will add it to exclusion list)
23:29:35.40 +53:27:37.2 -- not an asteroid (will add it to exclusion list)
23:45:36.35 +50:06:48.3 -- not an asteroid (will add it to exclusion list)
23:32:07.61 +51:53:29.5 -- not an asteroid (will add it to exclusion list)
23:41:05.57 +55:10:25.8 -- not an asteroid (will add it to exclusion list)
23:23:00.98 +49:26:22.2 -- not an asteroid (will add it to exclusion list)
23:16:55.27 +56:25:16.9 -- not an asteroid (will add it to exclusion list)
23:11:50.98 +56:02:39.9 -- not an asteroid (will add it to exclusion list)
00:25:59.25 +53:55:33.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:02:21.53 +52:42:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:31.58 +52:54:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:25.34 +56:43:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:35.28 +53:09:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:34.62 +54:54:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:15.80 +50:53:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:36.26 +55:01:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:57.56 +52:30:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:57.79 +53:09:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:41.39 +53:05:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:05.15 +53:32:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:29.89 +51:35:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:15.52 +53:28:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:31.73 +53:26:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:32.47 +52:19:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:39.55 +50:02:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:07.36 +54:58:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:21.70 +52:13:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:02.75 +54:10:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:11.56 +50:01:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:35.21 +52:01:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:49.81 +56:38:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:35.35 +52:46:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:38.27 +54:57:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:39.50 +56:53:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:44.77 +51:40:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:26.81 +50:19:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:11.91 +53:08:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:38.78 +53:48:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:46.28 +52:31:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:49.15 +50:44:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:55.99 +51:39:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:59.44 +49:51:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:09.79 +50:03:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:16.13 +56:02:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:18.03 +55:02:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:19.05 +53:07:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:25.43 +53:02:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:33.45 +54:59:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:40.06 +52:14:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:13.10 +57:50:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:14.21 +56:19:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:18.60 +57:02:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:23.60 +51:25:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:26.62 +49:47:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:29.39 +52:44:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:35.04 +53:03:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:42.72 +53:39:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:56.73 +54:53:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:58.75 +53:30:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:01.69 +50:32:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:09.60 +50:01:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:11.77 +53:11:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:15.79 +49:56:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:22.11 +56:40:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:36.10 +56:44:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:39.34 +50:08:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:39.72 +50:29:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:44.49 +51:17:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:04.80 +51:18:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:08.44 +52:18:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:11.65 +50:41:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:26.56 +54:51:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:32.75 +57:40:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:34.70 +53:55:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:42.19 +52:22:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:43.91 +51:43:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:44.46 +51:33:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:47.94 +49:56:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:51.26 +57:01:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:51.47 +49:58:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:52.20 +52:16:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:58.34 +51:55:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:08.60 +53:27:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:24.11 +51:48:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:27.48 +52:05:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:43.80 +54:00:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:47.25 +53:49:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:50.70 +50:44:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:54.83 +52:26:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:00.51 +52:22:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:08.05 +51:41:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:10.51 +54:55:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:16.64 +54:40:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:16.93 +52:15:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:18.69 +51:09:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:27.38 +50:49:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:43.15 +54:48:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:54.66 +54:13:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:01.91 +51:22:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:10.45 +52:54:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:17.09 +52:50:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:25.25 +51:23:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:26.27 +50:18:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:29.93 +51:14:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:40.91 +50:29:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:06.20 +51:46:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:25.61 +50:26:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:32.61 +55:48:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:37.31 +55:20:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:39.91 +53:29:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:42.53 +53:02:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:47.89 +51:26:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:50.32 +50:48:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:52.33 +53:12:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:54.91 +50:22:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:02.78 +55:28:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:09.96 +50:15:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:17.17 +51:18:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:19.22 +49:57:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:23.63 +50:19:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:24.90 +52:58:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:26.36 +53:32:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:26.76 +55:37:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:27.31 +57:21:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:27.91 +57:11:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:29.14 +53:23:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:32.66 +50:12:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:33.64 +50:28:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:40.29 +55:59:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:47.09 +56:08:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:54.84 +54:39:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:55.10 +50:43:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:00.01 +56:14:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:01.16 +55:19:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:02.99 +53:23:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:08.57 +56:25:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:08.99 +56:12:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:12.60 +56:31:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:14.90 +49:51:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:18.10 +57:04:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:19.19 +57:25:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:19.81 +55:26:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:21.82 +52:37:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:25.68 +49:53:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:27.09 +50:00:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:28.39 +53:44:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:28.88 +50:20:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:29.74 +55:20:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:30.01 +49:43:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:34.05 +51:58:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:40.54 +49:43:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:48.36 +53:57:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:48.45 +51:44:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:53.58 +53:52:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:59.25 +53:55:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:59.87 +50:55:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:00.38 +51:13:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:03.61 +57:31:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:06.36 +49:46:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:07.92 +49:44:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:09.86 +50:22:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:21.17 +50:40:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:25.79 +51:06:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:27.67 +52:48:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:28.07 +52:02:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:29.58 +57:34:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:30.66 +57:24:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:32.41 +53:23:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:35.77 +52:23:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:38.20 +51:44:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:39.90 +55:47:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:45.25 +51:29:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:48.60 +52:36:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:48.99 +50:20:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:50.34 +50:01:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:51.01 +49:46:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:53.21 +56:55:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:06.63 +50:36:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:06.84 +53:36:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:11.52 +51:41:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:12.40 +54:18:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:12.85 +50:07:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:16.60 +50:21:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:16.82 +49:54:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:18.50 +51:50:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:19.19 +57:11:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:23.78 +54:00:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:32.04 +49:53:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:39.18 +50:22:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:39.88 +50:01:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:47.97 +52:08:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:53.14 +51:36:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:57.22 +51:38:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:57.87 +53:27:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:57.97 +51:44:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:04.73 +57:36:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:05.07 +52:23:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:15.30 +52:44:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:22.86 +57:29:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:26.64 +52:38:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:27.49 +52:13:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:32.21 +51:40:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:36.32 +52:45:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:36.78 +57:23:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:36.83 +57:13:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:43.64 +53:35:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:44.79 +55:16:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:49.63 +53:12:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:50.00 +52:17:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:02.41 +55:22:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:07.59 +52:19:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:26.67 +55:24:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:45.46 +55:26:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:52.44 +53:42:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:00.23 +57:34:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:02.61 +57:31:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:06.96 +55:40:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:07.09 +56:57:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:18.77 +56:07:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:26.43 +55:57:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:30.72 +55:12:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:39.20 +57:46:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:41.22 +55:28:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:54.29 +55:16:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:59.57 +57:25:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:04.51 +55:56:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:08.08 +57:01:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:11.03 +55:35:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:11.54 +56:01:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:20.89 +57:06:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:44.06 +56:11:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:58.07 +57:30:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:02.90 +57:43:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:50.17 +56:02:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:50.98 +56:02:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:08.93 +56:57:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:38.24 +57:25:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:55.27 +56:25:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:59.96 +56:24:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:45.74 +54:26:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:00.98 +49:26:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:39.95 +49:26:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:20.30 +56:49:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:35.40 +53:27:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:49.50 +55:35:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:07.61 +51:53:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:13.83 +53:34:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:26.19 +50:19:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:38.52 +51:42:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:05.57 +55:10:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:36.35 +50:06:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:35.12 +54:28:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:41.61 +54:28:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:33.87 +55:08:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:10.53 +50:21:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:40.10 +50:22:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:55.73 +56:31:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:17.80 +56:36:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:06.71 +51:17:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:09.66 +50:28:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:30.50 +54:23:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:46.81 +52:11:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:47.87 +56:36:56.2 -- 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)
00:02:21.53 +52:42:49.5 -- not a known variable star
00:04:31.58 +52:54:29.4 -- not a known variable star
00:05:25.34 +56:43:01.1 -- not a known variable star
00:05:35.28 +53:09:22.8 -- not a known variable star
00:06:34.62 +54:54:42.1 -- not a known variable star
00:07:15.80 +50:53:28.8 -- a known variable star
00:07:36.26 +55:01:28.7 -- a known variable star
00:07:57.56 +52:30:05.1 -- not a known variable star
00:07:57.79 +53:09:53.4 -- not a known variable star
00:08:41.39 +53:05:02.5 -- not a known variable star
00:09:05.15 +53:32:52.1 -- a known variable star
00:09:29.89 +51:35:56.4 -- not a known variable star
00:10:15.52 +53:28:38.1 -- not a known variable star
00:10:31.73 +53:26:21.2 -- not a known variable star
00:10:32.47 +52:19:31.2 -- not a known variable star
00:10:39.55 +50:02:31.4 -- not a known variable star
00:11:07.36 +54:58:20.1 -- not a known variable star
00:11:21.70 +52:13:52.0 -- not a known variable star
00:12:02.75 +54:10:32.6 -- not a known variable star
00:12:11.56 +50:01:07.2 -- not a known variable star
00:12:35.21 +52:01:41.7 -- not a known variable star
00:12:49.81 +56:38:44.7 -- not a known variable star
00:13:35.35 +52:46:38.3 -- not a known variable star
00:13:38.27 +54:57:36.2 -- not a known variable star
00:13:39.50 +56:53:46.2 -- not a known variable star
00:13:44.77 +51:40:32.5 -- a known variable star
00:14:26.81 +50:19:37.6 -- not a known variable star
00:15:11.91 +53:08:55.7 -- not a known variable star
00:15:38.78 +53:48:04.1 -- not a known variable star
00:15:46.28 +52:31:20.1 -- not a known variable star
00:15:49.15 +50:44:30.1 -- not a known variable star
00:15:55.99 +51:39:55.6 -- not a known variable star
00:15:59.44 +49:51:23.2 -- not a known variable star
00:16:09.79 +50:03:00.1 -- not a known variable star
00:16:16.13 +56:02:21.4 -- not a known variable star
00:16:18.03 +55:02:57.1 -- not a known variable star
00:16:19.05 +53:07:30.1 -- not a known variable star
00:16:25.43 +53:02:33.7 -- not a known variable star
00:16:33.45 +54:59:15.9 -- not a known variable star
00:16:40.06 +52:14:35.6 -- not a known variable star
00:17:13.10 +57:50:20.7 -- a known variable star
00:17:14.21 +56:19:32.5 -- not a known variable star
00:17:18.60 +57:02:33.1 -- not a known variable star
00:17:23.60 +51:25:21.8 -- not a known variable star
00:17:26.62 +49:47:25.8 -- not a known variable star
00:17:29.39 +52:44:47.7 -- not a known variable star
00:17:35.04 +53:03:34.7 -- not a known variable star
00:17:42.72 +53:39:39.1 -- not a known variable star
00:17:56.73 +54:53:04.5 -- not a known variable star
00:17:58.75 +53:30:39.8 -- not a known variable star
00:18:01.69 +50:32:50.2 -- not a known variable star
00:18:09.60 +50:01:26.6 -- not a known variable star
00:18:11.77 +53:11:42.1 -- not a known variable star
00:18:15.79 +49:56:31.0 -- a known variable star
00:18:22.11 +56:40:04.9 -- not a known variable star
00:18:36.10 +56:44:54.8 -- not a known variable star
00:18:39.34 +50:08:44.0 -- not a known variable star
00:18:39.72 +50:29:11.2 -- not a known variable star
00:18:44.49 +51:17:52.0 -- not a known variable star
00:19:04.80 +51:18:58.4 -- not a known variable star
00:19:08.44 +52:18:48.1 -- not a known variable star
00:19:11.65 +50:41:05.8 -- not a known variable star
00:19:26.56 +54:51:21.8 -- not a known variable star
00:19:32.75 +57:40:55.6 -- not a known variable star
00:19:34.70 +53:55:07.7 -- a known variable star
00:19:42.19 +52:22:46.0 -- not a known variable star
00:19:43.91 +51:43:50.6 -- not a known variable star
00:19:44.46 +51:33:12.2 -- not a known variable star
00:19:47.94 +49:56:35.6 -- not a known variable star
00:19:51.26 +57:01:50.4 -- not a known variable star
00:19:51.47 +49:58:31.6 -- a known variable star
00:19:52.20 +52:16:55.0 -- not a known variable star
00:19:58.34 +51:55:30.9 -- not a known variable star
00:20:08.60 +53:27:53.1 -- not a known variable star
00:20:24.11 +51:48:24.3 -- not a known variable star
00:20:27.48 +52:05:03.1 -- a known variable star
00:20:43.80 +54:00:53.8 -- not a known variable star
00:20:47.25 +53:49:55.8 -- not a known variable star
00:20:50.70 +50:44:15.7 -- not a known variable star
00:20:54.83 +52:26:46.7 -- not a known variable star
00:21:00.51 +52:22:38.5 -- not a known variable star
00:21:08.05 +51:41:04.5 -- not a known variable star
00:21:10.51 +54:55:18.0 -- not a known variable star
00:21:16.64 +54:40:28.1 -- not a known variable star
00:21:16.93 +52:15:27.7 -- not a known variable star
00:21:18.69 +51:09:17.7 -- not a known variable star
00:21:27.38 +50:49:24.9 -- not a known variable star
00:21:43.15 +54:48:13.6 -- not a known variable star
00:21:54.66 +54:13:19.1 -- not a known variable star
00:22:01.91 +51:22:31.0 -- not a known variable star
00:22:10.45 +52:54:58.0 -- not a known variable star
00:22:17.09 +52:50:24.0 -- not a known variable star
00:22:25.25 +51:23:55.3 -- not a known variable star
00:22:26.27 +50:18:54.7 -- not a known variable star
00:22:29.93 +51:14:18.7 -- not a known variable star
00:22:40.91 +50:29:36.0 -- a known variable star
00:23:06.20 +51:46:47.4 -- not a known variable star
00:23:25.61 +50:26:02.3 -- not a known variable star
00:23:32.61 +55:48:00.5 -- not a known variable star
00:23:37.31 +55:20:26.7 -- not a known variable star
00:23:39.91 +53:29:32.0 -- not a known variable star
00:23:42.53 +53:02:06.5 -- not a known variable star
00:23:47.89 +51:26:19.6 -- not a known variable star
00:23:50.32 +50:48:29.0 -- a known variable star
00:23:52.33 +53:12:05.9 -- not a known variable star
00:23:54.91 +50:22:50.0 -- not a known variable star
00:24:02.78 +55:28:19.1 -- not a known variable star
00:24:09.96 +50:15:32.5 -- not a known variable star
00:24:17.17 +51:18:55.2 -- a known variable star
00:24:19.22 +49:57:03.6 -- not a known variable star
00:24:23.63 +50:19:40.3 -- not a known variable star
00:24:24.90 +52:58:26.1 -- not a known variable star
00:24:26.36 +53:32:29.6 -- not a known variable star
00:24:26.76 +55:37:43.0 -- not a known variable star
00:24:27.31 +57:21:46.5 -- a known variable star
00:24:27.91 +57:11:49.9 -- not a known variable star
00:24:29.14 +53:23:18.7 -- not a known variable star
00:24:32.66 +50:12:45.2 -- not a known variable star
00:24:33.64 +50:28:22.8 -- not a known variable star
00:24:40.29 +55:59:40.1 -- not a known variable star
00:24:47.09 +56:08:45.9 -- not a known variable star
00:24:54.84 +54:39:08.3 -- not a known variable star
00:24:55.10 +50:43:56.9 -- not a known variable star
00:25:00.01 +56:14:23.1 -- not a known variable star
00:25:01.16 +55:19:54.8 -- a known variable star
00:25:02.99 +53:23:18.1 -- not a known variable star
00:25:08.57 +56:25:14.8 -- not a known variable star
00:25:08.99 +56:12:31.0 -- not a known variable star
00:25:12.60 +56:31:45.4 -- not a known variable star
00:25:14.90 +49:51:28.7 -- not a known variable star
00:25:18.10 +57:04:42.7 -- a known variable star
00:25:19.19 +57:25:08.3 -- not a known variable star
00:25:19.81 +55:26:51.3 -- not a known variable star
00:25:21.82 +52:37:58.0 -- not a known variable star
00:25:25.68 +49:53:23.2 -- not a known variable star
00:25:27.09 +50:00:26.5 -- not a known variable star
00:25:28.39 +53:44:31.2 -- not a known variable star
00:25:28.88 +50:20:21.6 -- not a known variable star
00:25:29.74 +55:20:20.4 -- not a known variable star
00:25:30.01 +49:43:57.0 -- not a known variable star
00:25:34.05 +51:58:55.4 -- not a known variable star
00:25:40.54 +49:43:18.4 -- not a known variable star
00:25:48.36 +53:57:27.4 -- not a known variable star
00:25:48.45 +51:44:26.3 -- not a known variable star
00:25:53.58 +53:52:55.2 -- not a known variable star
00:25:59.25 +53:55:33.9 -- not a known variable star
00:25:59.87 +50:55:09.0 -- not a known variable star
00:26:00.38 +51:13:40.9 -- not a known variable star
00:26:03.61 +57:31:00.9 -- not a known variable star
00:26:06.36 +49:46:55.2 -- not a known variable star
00:26:07.92 +49:44:43.2 -- not a known variable star
00:26:09.86 +50:22:56.2 -- not a known variable star
00:26:21.17 +50:40:28.0 -- not a known variable star
00:26:25.79 +51:06:49.6 -- not a known variable star
00:26:27.67 +52:48:18.2 -- not a known variable star
00:26:28.07 +52:02:02.1 -- not a known variable star
00:26:29.58 +57:34:31.3 -- not a known variable star
00:26:30.66 +57:24:44.4 -- not a known variable star
00:26:32.41 +53:23:37.5 -- not a known variable star
00:26:35.77 +52:23:53.9 -- not a known variable star
00:26:38.20 +51:44:56.0 -- not a known variable star
00:26:39.90 +55:47:37.7 -- not a known variable star
00:26:45.25 +51:29:25.7 -- not a known variable star
00:26:48.60 +52:36:36.7 -- a known variable star
00:26:48.99 +50:20:31.3 -- not a known variable star
00:26:50.34 +50:01:56.9 -- not a known variable star
00:26:51.01 +49:46:16.4 -- not a known variable star
00:26:53.21 +56:55:11.3 -- not a known variable star
00:27:06.63 +50:36:29.3 -- not a known variable star
00:27:06.84 +53:36:16.6 -- not a known variable star
00:27:11.52 +51:41:47.4 -- not a known variable star
00:27:12.40 +54:18:54.6 -- not a known variable star
00:27:12.85 +50:07:02.8 -- not a known variable star
00:27:16.60 +50:21:07.3 -- not a known variable star
00:27:16.82 +49:54:40.3 -- a known variable star
00:27:18.50 +51:50:42.3 -- not a known variable star
00:27:19.19 +57:11:04.1 -- not a known variable star
00:27:23.78 +54:00:55.1 -- not a known variable star
00:27:32.04 +49:53:18.8 -- not a known variable star
00:27:39.18 +50:22:51.4 -- not a known variable star
00:27:39.88 +50:01:01.5 -- not a known variable star
00:27:47.97 +52:08:25.3 -- a known variable star
00:27:53.14 +51:36:40.1 -- a known variable star
00:27:57.22 +51:38:49.2 -- not a known variable star
00:27:57.87 +53:27:54.7 -- not a known variable star
00:27:57.97 +51:44:12.5 -- not a known variable star
00:28:04.73 +57:36:04.4 -- not a known variable star
00:28:05.07 +52:23:38.9 -- not a known variable star
00:28:15.30 +52:44:18.1 -- not a known variable star
00:28:22.86 +57:29:15.3 -- not a known variable star
00:28:26.64 +52:38:28.9 -- a known variable star
00:28:27.49 +52:13:56.6 -- not a known variable star
00:28:32.21 +51:40:59.2 -- not a known variable star
00:28:36.32 +52:45:09.1 -- not a known variable star
00:28:36.78 +57:23:02.9 -- a known variable star
00:28:36.83 +57:13:19.5 -- not a known variable star
00:28:43.64 +53:35:06.8 -- not a known variable star
00:28:44.79 +55:16:06.5 -- not a known variable star
00:28:49.63 +53:12:01.3 -- not a known variable star
00:28:50.00 +52:17:32.3 -- not a known variable star
00:29:02.41 +55:22:39.7 -- not a known variable star
00:29:07.59 +52:19:12.8 -- not a known variable star
00:29:26.67 +55:24:39.1 -- not a known variable star
00:29:45.46 +55:26:25.4 -- a known variable star
00:29:52.44 +53:42:26.9 -- not a known variable star
00:30:00.23 +57:34:37.8 -- not a known variable star
00:30:02.61 +57:31:36.2 -- not a known variable star
00:30:06.96 +55:40:15.5 -- not a known variable star
00:30:07.09 +56:57:05.6 -- not a known variable star
00:30:18.77 +56:07:42.4 -- not a known variable star
00:30:26.43 +55:57:29.1 -- not a known variable star
00:30:30.72 +55:12:22.2 -- not a known variable star
00:30:39.20 +57:46:18.9 -- a known variable star
00:30:41.22 +55:28:16.4 -- not a known variable star
00:30:54.29 +55:16:20.2 -- not a known variable star
00:30:59.57 +57:25:04.4 -- a known variable star
00:31:04.51 +55:56:03.4 -- not a known variable star
00:31:08.08 +57:01:57.2 -- not a known variable star
00:31:11.03 +55:35:42.6 -- not a known variable star
00:31:11.54 +56:01:45.2 -- not a known variable star
00:31:20.89 +57:06:28.4 -- not a known variable star
00:31:44.06 +56:11:45.7 -- not a known variable star
00:31:58.07 +57:30:55.6 -- not a known variable star
00:32:02.90 +57:43:25.8 -- not a known variable star
23:11:50.17 +56:02:36.5 -- not a known variable star
23:11:50.98 +56:02:39.9 -- not a known variable star
23:13:08.93 +56:57:55.6 -- not a known variable star
23:16:38.24 +57:25:37.4 -- not a known variable star
23:16:55.27 +56:25:16.9 -- not a known variable star
23:16:59.96 +56:24:23.4 -- not a known variable star
23:21:45.74 +54:26:17.6 -- not a known variable star
23:23:00.98 +49:26:22.2 -- not a known variable star
23:23:39.95 +49:26:42.9 -- a known variable star
23:25:20.30 +56:49:19.5 -- not a known variable star
23:29:35.40 +53:27:37.2 -- not a known variable star
23:31:49.50 +55:35:28.2 -- a known variable star
23:32:07.61 +51:53:29.5 -- not a known variable star
23:32:13.83 +53:34:05.7 -- not a known variable star
23:33:26.19 +50:19:13.1 -- not a known variable star
23:36:38.52 +51:42:55.0 -- not a known variable star
23:41:05.57 +55:10:25.8 -- not a known variable star
23:45:36.35 +50:06:48.3 -- not a known variable star
23:46:35.12 +54:28:36.8 -- not a known variable star
23:46:41.61 +54:28:42.6 -- a known variable star
23:49:33.87 +55:08:18.7 -- not a known variable star
23:52:10.53 +50:21:19.9 -- not a known variable star
23:52:40.10 +50:22:49.0 -- not a known variable star
23:54:55.73 +56:31:16.7 -- not a known variable star
23:55:17.80 +56:36:24.9 -- not a known variable star
23:57:06.71 +51:17:45.6 -- not a known variable star
23:57:09.66 +50:28:26.1 -- not a known variable star
23:57:30.50 +54:23:42.9 -- not a known variable star
23:57:46.81 +52:11:11.3 -- not a known variable star
23:57:47.87 +56:36:56.2 -- not a known variable star
Found 227 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
254 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 254 (excluding asteroids and hot pixels, 227 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)2461234.78823116 -observatory V36
07:24:19.69 +17:06:52.4 Mercury (5.6mag)
10:23:51.59 +11:22:44.7 Venus (-4.1mag)
04:32:52.86 +21:46:25.3 Mars (1.3mag)
08:19:20.81 +20:02:59.6 Jupiter (-1.8mag)
00:56:08.73 +03:21:27.3 Saturn (0.7mag)
04:07:47.26 +20:46:32.9 Uranus (5.8mag)
00:17:00.19 +00:20:22.7 Neptune (7.7mag)
20:30:38.63 -23:19:18.3 Pluto (14.4mag)
06:22:24.60 +26:43:55.5 Moon (-8.5mag)
-rw-r--r-- 1 apache apache 361 Jul 13 08:43 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461234.78823116:
08:19:16.38 +20:03:17.5 Io (6.1mag)
08:19:13.99 +20:03:26.8 Europa (6.3mag)
08:19:11.21 +20:03:33.6 Ganymede (5.6mag)
08:19:24.94 +20:02:40.1 Callisto (6.8mag)
08:17:44.28 +19:48:24.4 Himalia (15.7mag)
08:19:25.52 +20:02:42.2 Thebe (16.6mag)
08:17:05.07 +19:52:13.3 Elara (17.6mag)
08:22:58.40 +19:55:35.4 Pasiphae (17.8mag)
08:24:08.56 +20:08:30.2 Carme (19.0mag)
00:56:10.83 +03:20:56.5 Titan (8.5mag)
00:56:11.68 +03:21:33.1 Rhea (9.8mag)
00:55:35.13 +03:20:03.4 Iapetus (11.2mag)
00:56:05.17 +03:21:57.1 Hyperion (14.5mag)
00:56:05.53 +03:18:15.4 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 13 08:43 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461234.78823116:
17:50:20.43 -32:21:22.0 JWST
17:01:21.84 +43:49:01.3 Chandra
09:29:38.39 -53:50:21.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 13 08:43 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461234.78823116 -observatory V36
02:40:25.69 +14:46:31.2 17.9mag P/1996 R2 (Lagerkvist)
18:15:42.46 -34:26:27.2 13.7mag P/2010 H2 (Vales)
06:28:36.77 -68:11:16.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:01:49.39 +32:29:49.5 17.6mag C/2017 K2 (PANSTARRS)
02:03:58.67 +13:43:20.5 15.5mag P/2021 N1 (ZTF)
22:57:44.82 +32:16:35.2 17.3mag C/2022 E2 (ATLAS)
06:15:44.65 +26:53:58.5 16.7mag C/2022 N2 (PANSTARRS)
09:58:04.70 +29:38:57.8 16.9mag C/2022 QE78 (ATLAS)
09:11:38.03 +05:03:14.7 17.8mag C/2022 R6 (PANSTARRS)
18:05:26.52 +21:10:40.9 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:19.01 -11:27:22.6 17.7mag P/2023 B1 (PANSTARRS)
21:45:39.61 +67:35:40.8 17.8mag C/2023 H5 (Lemmon)
16:25:11.03 -10:23:05.2 13.9mag C/2023 R1 (PANSTARRS)
08:05:45.62 +65:52:02.8 17.9mag C/2024 A1 (ATLAS)
07:36:39.05 +30:09:08.1 14.7mag C/2024 E1 (Wierzchos)
15:14:56.18 +15:24:09.3 17.6mag C/2024 G6 (ATLAS)
19:37:33.12 +39:57:20.3 13.8mag C/2024 J3 (ATLAS)
21:44:30.15 +46:26:23.8 17.8mag C/2024 R4 (PANSTARRS)
04:52:24.31 -13:39:55.6 15.7mag C/2024 T5 (ATLAS)
06:36:59.83 +28:34:48.2 18.0mag C/2025 J1 (Borisov)
07:16:22.83 -13:09:11.5 16.6mag C/2025 R3 (PANSTARRS)
09:59:30.90 +22:18:34.3 17.6mag C/2025 V2 (Rankin)
12:45:37.27 +03:48:37.4 17.1mag C/2025 Y1 (ATLAS)
16:43:46.38 +79:09:53.1 17.3mag C/2026 A2 (Bok)
02:49:20.98 +45:21:56.9 16.7mag C/2026 B2 (Sun-Gao)
11:27:23.91 +05:03:31.5 17.0mag A/2026 E1
21:23:38.09 -16:08:41.3 7.2mag 10P/Tempel
11:14:50.57 -02:00:51.2 16.2mag 29P/Schwassmann-Wachmann
04:04:23.89 +29:52:17.1 17.9mag 47P/Ashbrook-Jackson
10:14:12.55 +13:04:28.6 17.0mag 63P/Wild
00:49:36.24 -05:03:46.4 15.5mag 65P/Gunn
04:34:29.99 +20:19:33.5 13.7mag 78P/Gehrels
02:27:03.25 +11:00:39.1 16.3mag 88P/Howell
06:44:15.30 +30:21:16.3 15.7mag 93P/Lovas
04:30:32.95 +31:14:06.6 16.8mag 114P/Wiseman-Skiff
08:15:52.37 +30:22:20.4 15.2mag 123P/West-Hartley
10:53:36.98 -00:00:25.8 16.8mag 124P/Mrkos
04:56:26.64 +20:53:41.4 16.2mag 128P/Shoemaker-Holt
05:41:47.42 +19:41:16.8 17.8mag 131P/Mueller
00:02:18.75 +03:02:48.6 17.9mag 139P/Vaisala-Oterma
07:24:18.45 +16:22:53.4 15.9mag 141P-D/Machholz
03:18:03.59 -20:51:50.8 15.3mag 161P/Hartley-IRAS
05:43:38.87 +34:34:04.5 15.4mag 162P/SidingSpring
18:56:33.25 +16:56:10.0 14.5mag 169P/NEAT
01:48:01.29 +07:55:21.9 17.7mag 220P/McNaught
16:35:37.78 -08:30:18.5 17.1mag 235P/LINEAR
08:51:28.10 +33:01:35.5 17.9mag 240P/NEAT
20:40:51.10 -50:12:06.6 17.8mag 259P/Garradd
02:07:32.38 +13:28:07.9 15.6mag 260P/McNaught
05:46:08.67 +37:04:15.3 17.4mag 295P/LINEAR
15:06:29.50 +05:47:36.5 17.6mag 391P/Kowalski
08:37:14.60 +19:33:25.0 17.9mag 450P/LONEOS
07:56:22.49 +38:58:18.8 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 13 08:43 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 13 08:43 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 13 08:43 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:46:18.966 +00:29:18.31 AT 2026tpp 2026-02-27.64 22.03
11:11:05.252 -20:09:49.14 AT 2026tpo 2026-04-19.33 21.35
08:27:14.950 +07:35:58.82 AT 2026tpn 2026-03-09.32 21.47
14:00:01.608 -17:41:28.55 AT 2026tpm 2026-06-07.29 21.68
12:16:26.621 +11:00:26.08 AT 2026tpl 2026-02-16.62 21.16
15:25:29.604 -15:53:31.26 AT 2026tpk 2026-06-13.37 20.93
13:24:42.561 -06:22:23.48 AT 2026tpj 2026-01-20.63 20.87
15:50:59.060 +06:20:09.76 AT 2026tpi 2026-06-15.46 21.35
10:47:25.526 -03:49:23.63 AT 2026tph 2026-01-16.49 21.64
13:02:15.361 +45:51:35.20 AT 2026tpg 2026-01-08.63 20.9
10:13:04.585 -02:08:41.00 AT 2026tpf 2026-04-21.29 20.91
12:56:24.797 +39:54:51.89 AT 2026tpe 2026-02-12.65 22.32
12:17:06.882 -15:52:23.32 AT 2026tpd 2026-05-17.30 21.49
09:57:03.429 +14:12:08.48 AT 2026tpc 2026-04-06.25 21.31
12:58:16.246 -16:08:31.20 AT 2026tpb 2026-02-26.58 21.35
08:11:52.444 +10:55:48.58 AT 2026tpa 2026-01-28.35 21.11
21:33:46.265 +27:03:56.69 AT 2026toz 2026-06-22.49 21.16
15:31:46.821 +19:25:51.54 AT 2026toy 2026-04-21.55 21.27
10:44:05.178 +12:45:21.54 AT 2026tox 2026-01-16.61 21.73
15:35:47.080 -21:09:58.65 AT 2026tow 2026-02-26.62 21.35
-rw-r--r-- 1 apache apache 30K Jul 13 08:43 tns_transients_list.txt
