This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg
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 10.1985 2461231.6985 9.28 00:35:09.93 +49:02:17.0
120.18765 -13.74697 galactic Cas Second-epoch detections are separated by 3.8" and 5.1 pix
The object was found in VSX 3" ASASSN-V J003509.93+490214.3
Type: SR
# Max. Min./Amp. JD0 Period
11.390 g Y 0.790 g 2458428.85500 97.570000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:09.93 +49:02:17.0: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:09.93 +49:02:17.0: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 09.93 +49 02 17.0 9.3 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 J003509.93+490214.3,2461231.6985,9.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J003509.93+490214.3 20260710.1985 9.28CV 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 10.1985 2461231.6985 9.61 00:34:23.57 +49:19:33.0
120.07772 -13.45143 galactic Cas Second-epoch detections are separated by 3.2" and 5.0 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 | 00:34:23.57 +49:19:33.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:23.57 +49:19:33.0: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:23.57 +49:19:33.0: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 23.57 +49 19 33.0 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
target,2461231.6985,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 9.61CV 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 10.1985 2461231.6985 9.72 00:27:48.38 +48:44:52.3
118.92203 -13.93981 galactic Cas Second-epoch detections are separated by 4.4" and 5.0 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 | 00:27:48.38 +48:44:52.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:48.38 +48:44:52.3: 13.54 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:48.38 +48:44:52.3: 14.54 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 10.1985* 00 27 48.38 +48 44 52.3 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,9.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 9.72CV 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 10.1985 2461231.6985 9.78 00:29:36.73 +48:43:49.9
119.22594 -13.98411 galactic Cas Second-epoch detections are separated by 4.8" and 5.0 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 | 00:29:36.73 +48:43:49.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:36.73 +48:43:49.9: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:36.73 +48:43:49.9: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 29 36.73 +48 43 49.9 9.8 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,2461231.6985,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 9.78CV 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 10.1985 2461231.6985 9.82 00:46:53.36 +50:47:03.4
122.19671 -12.08098 galactic Cas Second-epoch detections are separated by 5.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:46:53.36 +50:47:03.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:53.36 +50:47:03.4: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:53.36 +50:47:03.4: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 53.36 +50 47 03.4 9.8 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,2461231.6985,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 9.82CV 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 10.1985 2461231.6985 9.97 00:33:15.80 +49:05:57.8
119.87207 -13.66435 galactic Cas Second-epoch detections are separated by 5.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:33:15.80 +49:05:57.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:15.80 +49:05:57.8: 15.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:15.80 +49:05:57.8: 15.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 33 15.80 +49 05 57.8 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.13 00:44:46.84 +50:46:19.3
121.85562 -12.08581 galactic Cas Second-epoch detections are separated by 4.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:44:46.84 +50:46:19.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:46.84 +50:46:19.3: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:46.84 +50:46:19.3: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 46.84 +50 46 19.3 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,2461231.6985,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.13CV 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 10.1985 2461231.6985 10.05 00:34:29.49 +49:19:02.2
120.09362 -13.46106 galactic Cas Second-epoch detections are separated by 2.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:34:29.49 +49:19:02.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:29.49 +49:19:02.2: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:29.49 +49:19:02.2: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 29.49 +49 19 02.2 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,2461231.6985,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.22 00:31:30.22 +49:04:17.1
119.57423 -13.67033 galactic Cas Second-epoch detections are separated by 6.1" and 5.0 pix
The object was found in VSX 1" Gaia DR3 391161951761028480
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.320 G 11.370 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:30.22 +49:04:17.1: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:30.22 +49:04:17.1: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 31 30.22 +49 04 17.1 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391161951761028480,2461231.6985,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391161951761028480 20260710.1985 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.12 00:37:47.79 +49:14:14.2
120.64196 -13.57381 galactic Cas Second-epoch detections are separated by 3.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:37:47.79 +49:14:14.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:47.79 +49:14:14.2: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:47.79 +49:14:14.2: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 37 47.79 +49 14 14.2 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,2461231.6985,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.12CV 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 10.1985 2461231.6985 10.30 00:34:30.75 +49:44:36.9
120.12667 -13.03595 galactic Cas Second-epoch detections are separated by 2.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:34:30.75 +49:44:36.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:30.75 +49:44:36.9: 15.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:30.75 +49:44:36.9: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 30.75 +49 44 36.9 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.19 23:11:31.33 +56:01:29.3
109.24518 -4.16887 galactic Cas Second-epoch detections are separated by 3.2" and 3.9 pix
The object was found in VSX 2" V0349 Cas
Type: SR
# Max. Min./Amp. JD0 Period
12.500 pg 14.200 pg 2428377.00000 70.790000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:11:31.33 +56:01:29.3: 14.81 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:11:31.33 +56:01:29.3: 14.70 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.75 +/- 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 10.1985* 23 11 31.33 +56 01 29.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0349 Cas,2461231.6985,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0349 Cas 20260710.1985 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.28 00:44:04.93 +49:03:55.9
121.69142 -13.78850 galactic Cas Second-epoch detections are separated by 8.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:44:04.93 +49:03:55.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:04.93 +49:03:55.9: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:04.93 +49:03:55.9: 14.92 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 04.93 +49 03 55.9 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.28CV 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 10.1985 2461231.6985 10.54 00:30:23.39 +48:54:32.5
119.37307 -13.81722 galactic Cas Second-epoch detections are separated by 4.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:30:23.39 +48:54:32.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:23.39 +48:54:32.5: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:23.39 +48:54:32.5: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 30 23.39 +48 54 32.5 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.54CV 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 10.1985 2461231.6985 10.60 00:32:51.85 +49:19:38.8
119.82239 -13.43213 galactic Cas Second-epoch detections are separated by 3.8" and 5.0 pix
The object was found in VSX 2" V0381 Cas
Type: EA/DM
# Max. Min./Amp. JD0 Period
10.200 pg 10.800 pg 2456970.43400 1.745957000000 B3
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:32:51.85 +49:19:38.8: 15.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:32:51.85 +49:19:38.8: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 32 51.85 +49 19 38.8 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
V0381 Cas,2461231.6985,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0381 Cas 20260710.1985 10.60CV 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 10.1985 2461231.6985 10.64 00:48:02.30 +50:47:44.6
122.38257 -12.07240 galactic Cas Second-epoch detections are separated by 7.2" 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 | 00:48:02.30 +50:47:44.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:02.30 +50:47:44.6: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:02.30 +50:47:44.6: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 48 02.30 +50 47 44.6 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,2461231.6985,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 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 10.1985 2461231.6985 10.66 00:27:08.02 +48:44:41.6
118.80801 -13.93215 galactic Cas Second-epoch detections are separated by 4.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:27:08.02 +48:44:41.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:08.02 +48:44:41.6: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:08.02 +48:44:41.6: 15.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 27 08.02 +48 44 41.6 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.70 00:32:49.72 +49:11:25.7
119.80601 -13.56830 galactic Cas Second-epoch detections are separated by 3.7" and 5.0 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 | 00:32:49.72 +49:11:25.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:32:49.72 +49:11:25.7: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:32:49.72 +49:11:25.7: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 32 49.72 +49 11 25.7 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.70CV 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 10.1985 2461231.6985 10.76 00:35:09.45 +49:16:34.4
120.20223 -13.50922 galactic Cas Second-epoch detections are separated by 2.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:35:09.45 +49:16:34.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:09.45 +49:16:34.4: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:09.45 +49:16:34.4: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 09.45 +49 16 34.4 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.76CV 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 10.1985 2461231.6985 10.77 00:45:27.46 +50:43:41.0
121.96398 -12.13245 galactic Cas Second-epoch detections are separated by 3.6" and 5.0 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 | 00:45:27.46 +50:43:41.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:27.46 +50:43:41.0: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:27.46 +50:43:41.0: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 27.46 +50 43 41.0 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.77CV 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 10.1985 2461231.6985 10.69 00:39:35.16 +48:51:40.5
120.92374 -13.96428 galactic Cas Second-epoch detections are separated by 2.9" 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 | 00:39:35.16 +48:51:40.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:35.16 +48:51:40.5: 13.33 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:35.16 +48:51:40.5: 13.46 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 10.1985* 00 39 35.16 +48 51 40.5 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.69CV 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 10.1985 2461231.6985 11.37 23:36:42.81 +52:12:23.4
111.46925 -8.99433 galactic Cas Second-epoch detections are separated by 1.0" and 4.4 pix
The object was found in VSX 2" ASASSN-V J233642.65+521224.3
Type: SR
# Max. Min./Amp. JD0 Period
12.110 V 12.750 V 2457581.00000 61.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:36:42.81 +52:12:23.4: 15.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:36:42.81 +52:12:23.4: 15.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 23 36 42.81 +52 12 23.4 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J233642.65+521224.3,2461231.6985,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J233642.65+521224.3 20260710.1985 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.68 23:10:51.78 +54:50:07.5
108.70690 -5.23452 galactic Cas Second-epoch detections are separated by 2.3" and 3.9 pix
The object was found in VSX 1" V0347 Cas
Type: SRA
# Max. Min./Amp. JD0 Period
14.000 pg 14.700 pg 2428359.00000 119.200000000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:10:51.78 +54:50:07.5: 14.61 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:10:51.78 +54:50:07.5: 14.42 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.50 +/- 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 10.1985* 23 10 51.78 +54 50 07.5 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
V0347 Cas,2461231.6985,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0347 Cas 20260710.1985 11.68CV 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 10.1985 2461231.6985 10.86 00:34:01.04 +49:25:53.0
120.02250 -13.34192 galactic Cas Second-epoch detections are separated by 3.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:34:01.04 +49:25:53.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:01.04 +49:25:53.0: 15.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:01.04 +49:25:53.0: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 01.04 +49 25 53.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.86 00:47:48.52 +50:46:25.5
122.34514 -12.09386 galactic Cas Second-epoch detections are separated by 5.7" 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 | 00:47:48.52 +50:46:25.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:48.52 +50:46:25.5: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:48.52 +50:46:25.5: 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 10.1985* 00 47 48.52 +50 46 25.5 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.94 00:33:37.46 +49:04:29.0
119.93092 -13.69320 galactic Cas Second-epoch detections are separated by 5.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:33:37.46 +49:04:29.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:37.46 +49:04:29.0: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:37.46 +49:04:29.0: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 33 37.46 +49 04 29.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.93 00:34:40.16 +48:54:44.3
120.09544 -13.86707 galactic Cas Second-epoch detections are separated by 6.6" and 5.2 pix
The object was found in VSX19" ZTF J003441.75+485454.1
Type: RS
# Max. Min./Amp. JD0 Period
15.694 g Y 0.082 g 2458272.05770 7.326816300000
ATTENTION: measured mag 10.93 is 4.7 mag brighter than the VSX record maximum brightness 15.61 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:40.16 +48:54:44.3: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:40.16 +48:54:44.3: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 40.16 +48 54 44.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J003441.75+485454.1,2461231.6985,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J003441.75+485454.1 20260710.1985 10.93CV 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 10.1985 2461231.6985 10.99 00:45:56.32 +51:07:56.6
122.05084 -11.72995 galactic Cas Second-epoch detections are separated by 1.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:45:56.32 +51:07:56.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:56.32 +51:07:56.6: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:56.32 +51:07:56.6: 14.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 56.32 +51 07 56.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.62 23:31:09.43 +54:16:19.7
111.28974 -6.77490 galactic Cas Second-epoch detections are separated by 1.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:31:09.43 +54:16:19.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:31:09.43 +54:16:19.7: 15.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:31:09.43 +54:16:19.7: 15.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 23 31 09.43 +54 16 19.7 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.81 23:16:48.80 +55:26:59.8
109.72792 -4.97724 galactic Cas Second-epoch detections are separated by 0.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:16:48.80 +55:26:59.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:16:48.80 +55:26:59.8: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:16:48.80 +55:26:59.8: 15.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 23 16 48.80 +55 26 59.8 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
target,2461231.6985,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 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 10.1985 2461231.6985 11.00 00:31:24.77 +49:05:00.4
119.55995 -13.65715 galactic Cas Second-epoch detections are separated by 6.7" and 5.0 pix
The object was found in VSX 4" Gaia DR3 391162157917417600
Type: ROT
# Max. Min./Amp. JD0 Period
10.660 G 10.700 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:24.77 +49:05:00.4: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:24.77 +49:05:00.4: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 31 24.77 +49 05 00.4 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391162157917417600,2461231.6985,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391162157917417600 20260710.1985 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.04 00:34:32.63 +48:57:00.3
120.07688 -13.82799 galactic Cas Second-epoch detections are separated by 4.5" and 5.0 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 | 00:34:32.63 +48:57:00.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:32.63 +48:57:00.3: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:32.63 +48:57:00.3: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 32.63 +48 57 00.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.09 00:34:57.81 +49:53:58.7
120.21180 -12.88508 galactic Cas Second-epoch detections are separated by 2.7" 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 | 00:34:57.81 +49:53:58.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:57.81 +49:53:58.7: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:57.81 +49:53:58.7: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 57.81 +49 53 58.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.85 00:25:03.08 +55:19:43.6
119.15384 -7.34929 galactic Cas Second-epoch detections are separated by 3.0" and 4.5 pix
The object was found in VSX 5" 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:03.08 +55:19:43.6: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:03.08 +55:19:43.6: 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 10.1985* 00 25 03.08 +55 19 43.6 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
WISE J002502.5+551944,2461231.6985,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260710.1985 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 10.1985 2461231.6985 12.12 23:17:32.89 +51:47:07.0
108.50804 -8.43763 galactic And Second-epoch detections are separated by 2.4" and 4.4 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 | 23:17:32.89 +51:47:07.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:17:32.89 +51:47:07.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:17:32.89 +51:47:07.0: 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 10.1985* 23 17 32.89 +51 47 07.0 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 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 10.1985 2461231.6985 11.88 00:04:11.16 +57:55:53.2
116.67380 -4.36501 galactic Cas Second-epoch detections are separated by 1.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:04:11.16 +57:55:53.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.725+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:04:11.16 +57:55:53.2: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:04:11.16 +57:55:53.2: 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 10.1985* 00 04 11.16 +57 55 53.2 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,2461231.6985,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.71 23:31:45.01 +54:09:37.0
111.33831 -6.90795 galactic Cas Second-epoch detections are separated by 1.3" and 4.7 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 | 23:31:45.01 +54:09:37.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:31:45.01 +54:09:37.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:31:45.01 +54:09:37.0: 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 10.1985* 23 31 45.01 +54 09 37.0 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
target,2461231.6985,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.48 00:30:29.22 +55:18:05.8
119.92775 -7.44788 galactic Cas Second-epoch detections are separated by 3.6" and 5.0 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 J007.6170+55.3085 | 00:30:29.22 +55:18:05.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:29.22 +55:18:05.8: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:29.22 +55:18:05.8: 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 10.1985* 00 30 29.22 +55 18 05.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J007.6170+55.3085,2461231.6985,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J007.6170+55.3085 20260710.1985 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 10.1985 2461231.6985 11.73 23:28:31.85 +53:36:18.8
110.70979 -7.28760 galactic Cas Second-epoch detections are separated by 3.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:31.85 +53:36:18.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:28:31.85 +53:36:18.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:28:31.85 +53:36:18.8: 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 10.1985* 23 28 31.85 +53 36 18.8 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.73CV 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 10.1985 2461231.6985 11.11 00:42:52.90 +52:06:34.0
121.59497 -10.74009 galactic Cas Second-epoch detections are separated by 6.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 415412123087149568 | 00:42:52.85 +52:06:41.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:52.90 +52:06:34.0: 13.27 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:52.90 +52:06:34.0: 12.66 +/- 0.21 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 10.1985* 00 42 52.90 +52 06 34.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415412123087149568,2461231.6985,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415412123087149568 20260710.1985 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.80 00:29:53.36 +50:13:53.1
119.40522 -12.49272 galactic Cas Second-epoch detections are separated by 0.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391744624204607360 | 00:29:51.65 +50:14:16.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.632+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:53.36 +50:13:53.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:53.36 +50:13:53.1: 13.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 29 53.36 +50 13 53.1 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 391744624204607360,2461231.6985,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391744624204607360 20260710.1985 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.03 00:43:19.98 +58:08:06.2
121.85875 -4.71980 galactic Cas Second-epoch detections are separated by 2.0" and 4.5 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 J010.8334+58.1350 | 00:43:19.98 +58:08:06.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.217+/-0.038 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:19.98 +58:08:06.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:19.98 +58:08:06.2: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 19.98 +58 08 06.2 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 J010.8334+58.1350,2461231.6985,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.8334+58.1350 20260710.1985 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.11 23:20:45.39 +53:43:33.9
109.65551 -6.79180 galactic Cas Second-epoch detections are separated by 4.5" and 4.1 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 1995765547479024384 | 23:20:40.68 +53:43:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:20:45.39 +53:43:33.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:20:45.39 +53:43:33.9: 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 10.1985* 23 20 45.39 +53 43 33.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995765547479024384,2461231.6985,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1995765547479024384 20260710.1985 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.77 00:31:10.05 +55:39:13.7
120.05324 -7.10460 galactic Cas Second-epoch detections are separated by 1.2" and 4.7 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 418262954885634432 | 00:31:11.84 +55:39:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:10.05 +55:39:13.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:10.05 +55:39:13.7: 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 10.1985* 00 31 10.05 +55 39 13.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 418262954885634432,2461231.6985,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 418262954885634432 20260710.1985 10.77CV 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 10.1985 2461231.6985 10.71 00:46:48.49 +58:10:11.1
122.31945 -4.69649 galactic Cas Second-epoch detections are separated by 4.5" and 4.6 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 425085184015674752 | 00:46:53.05 +58:10:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:48.49 +58:10:11.1: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:48.49 +58:10:11.1: 13.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 48.49 +58 10 11.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 425085184015674752,2461231.6985,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 425085184015674752 20260710.1985 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.85 00:53:07.27 +54:59:06.0
123.17568 -7.88595 galactic Cas Second-epoch detections are separated by 2.6" and 5.0 pix
The object was found in VSX 2" TYC 3659-550-1
Type: EW
# Max. Min./Amp. JD0 Period
11.410 V 11.500 V 2458097.98400 0.275862000000 F5
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:53:07.27 +54:59:06.0: 12.10 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:53:07.27 +54:59:06.0: 11.76 +/- 0.10 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 53 07.27 +54 59 06.0 9.8 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
TYC 3659-550-1,2461231.6985,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TYC 3659-550-1 20260710.1985 9.85CV 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 10.1985 2461231.6985 8.08 00:42:59.78 +51:05:48.6
121.57838 -11.75273 galactic Cas Second-epoch detections are separated by 4.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 415263658957212672 | 00:42:59.17 +51:05:52.2 (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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:59.78 +51:05:48.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:59.78 +51:05:48.6: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 59.78 +51 05 48.6 8.1 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
Large-amplitude variable Gaia DR2 415263658957212672,2461231.6985,8.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415263658957212672 20260710.1985 8.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 8.21 00:29:48.44 +49:15:04.0
119.30525 -13.46826 galactic Cas Second-epoch detections are separated by 3.5" and 5.0 pix
The object was found in VSX20" HAT-087-0048461
Type: VAR
# Max. Min./Amp. JD0 Period
15.261 V Y 0.065 V 0.184673000000
ATTENTION: measured mag 8.21 is 7.0 mag brighter than the VSX record maximum brightness 15.20 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:48.44 +49:15:04.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:48.44 +49:15:04.0: 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 10.1985* 00 29 48.44 +49 15 04.0 8.2 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
HAT-087-0048461,2461231.6985,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT-087-0048461 20260710.1985 8.21CV 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 10.1985 2461231.6985 8.52 00:57:24.04 +57:00:13.7
123.74792 -5.85850 galactic Cas Second-epoch detections are separated by 2.2" and 4.8 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 J014.3606+57.0129 | 00:57:24.26 +57:00:15.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.209+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:57:24.04 +57:00:13.7: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:57:24.04 +57:00:13.7: 13.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 57 24.04 +57 00 13.7 8.5 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 J014.3606+57.0129,2461231.6985,8.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014.3606+57.0129 20260710.1985 8.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 8.46 00:32:01.16 +49:19:09.0
119.68062 -13.42996 galactic Cas Second-epoch detections are separated by 7.2" and 5.0 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 391545642658633344 | 00:32:00.99 +49:19:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:32:01.16 +49:19:09.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:32:01.16 +49:19:09.0: 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 10.1985* 00 32 01.16 +49 19 09.0 8.5 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 391545642658633344,2461231.6985,8.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391545642658633344 20260710.1985 8.46CV 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 10.1985 2461231.6985 8.64 00:46:23.97 +49:40:43.6
122.09483 -13.18478 galactic Cas Second-epoch detections are separated by 5.5" and 5.2 pix
The object was found in VSX 4" Gaia DR3 414659271159337472
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
9.750 G 9.770 G 3.799620000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:23.97 +49:40:43.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:23.97 +49:40:43.6: 13.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 23.97 +49 40 43.6 8.6 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 414659271159337472,2461231.6985,8.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414659271159337472 20260710.1985 8.64CV 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 10.1985 2461231.6985 8.76 00:39:11.67 +49:08:18.6
120.87144 -13.68426 galactic Cas Second-epoch detections are separated by 5.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J009.7868+49.1411 | 00:39:11.36 +49:08:22.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:11.67 +49:08:18.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:11.67 +49:08:18.6: 13.01 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 11.67 +49 08 18.6 8.8 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 J009.7868+49.1411,2461231.6985,8.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.7868+49.1411 20260710.1985 8.76CV 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 10.1985 2461231.6985 8.99 00:30:54.04 +49:16:44.7
119.49042 -13.45538 galactic Cas Second-epoch detections are separated by 3.0" and 4.9 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 J007.7131+49.2785 | 00:30:53.96 +49:16:44.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.315+/-0.032 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:54.04 +49:16:44.7: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:54.04 +49:16:44.7: 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 10.1985* 00 30 54.04 +49 16 44.7 9.0 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 J007.7131+49.2785,2461231.6985,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J007.7131+49.2785 20260710.1985 8.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.12 00:43:48.42 +51:02:28.2
121.70659 -11.81243 galactic Cas Second-epoch detections are separated by 4.3" and 5.0 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 415251014574107776 | 00:43:47.55 +51:02:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:48.42 +51:02:28.2: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:48.42 +51:02:28.2: 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 10.1985* 00 43 48.42 +51 02 28.2 9.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415251014574107776,2461231.6985,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415251014574107776 20260710.1985 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.14 00:27:20.86 +48:44:02.2
118.84311 -13.94646 galactic Cas Second-epoch detections are separated by 3.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J006.8238+48.7333 | 00:27:20.70 +48:44:00.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:20.86 +48:44:02.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:20.86 +48:44:02.2: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 27 20.86 +48 44 02.2 9.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J006.8238+48.7333,2461231.6985,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J006.8238+48.7333 20260710.1985 9.14CV 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 10.1985 2461231.6985 9.21 00:45:30.28 +49:28:32.1
121.94125 -13.38475 galactic Cas Second-epoch detections are separated by 8.4" and 5.0 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 414652777168831360 | 00:45:30.00 +49:28:35.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:30.28 +49:28:32.1: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:30.28 +49:28:32.1: 13.18 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 30.28 +49 28 32.1 9.2 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 414652777168831360,2461231.6985,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414652777168831360 20260710.1985 9.21CV 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 10.1985 2461231.6985 9.16 00:39:40.72 +49:07:27.9
120.95217 -13.70212 galactic Cas Second-epoch detections are separated by 5.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J009.9065+49.1247 | 00:39:40.43 +49:07:31.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:40.72 +49:07:27.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:40.72 +49:07:27.9: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 40.72 +49 07 27.9 9.2 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 J009.9065+49.1247,2461231.6985,9.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.9065+49.1247 20260710.1985 9.16CV 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 10.1985 2461231.6985 9.44 00:46:31.50 +51:13:43.9
122.14669 -11.63540 galactic Cas Second-epoch detections are separated by 6.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J011.6214+51.2252 | 00:46:31.02 +51:13:49.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:31.50 +51:13:43.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:31.50 +51:13:43.9: 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 10.1985* 00 46 31.50 +51 13 43.9 9.4 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 J011.6214+51.2252,2461231.6985,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.6214+51.2252 20260710.1985 9.44CV 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 10.1985 2461231.6985 9.48 00:42:30.77 +50:54:50.5
121.49427 -11.93281 galactic Cas Second-epoch detections are separated by 2.1" and 5.0 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 J010.6128+50.9132 | 00:42:29.90 +50:54:56.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:30.77 +50:54:50.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:30.77 +50:54:50.5: 13.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 30.77 +50 54 50.5 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
ATO J010.6128+50.9132,2461231.6985,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.6128+50.9132 20260710.1985 9.48CV 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 10.1985 2461231.6985 9.34 00:39:56.30 +49:02:10.3
120.99167 -13.79223 galactic Cas Second-epoch detections are separated by 5.8" and 5.0 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 390642054557596416 | 00:39:55.89 +49:02:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:56.30 +49:02:10.3: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:56.30 +49:02:10.3: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 56.30 +49 02 10.3 9.3 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 390642054557596416,2461231.6985,9.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390642054557596416 20260710.1985 9.34CV 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 10.1985 2461231.6985 9.48 00:46:11.97 +50:44:47.5
122.08442 -12.11660 galactic Cas Second-epoch detections are separated by 5.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 415182123298541312 | 00:46:11.83 +50:44:51.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:11.97 +50:44:47.5: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:11.97 +50:44:47.5: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 11.97 +50 44 47.5 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
Gaia DR3 415182123298541312,2461231.6985,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415182123298541312 20260710.1985 9.48CV 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 10.1985 2461231.6985 9.38 00:46:04.86 +49:37:41.0
122.04081 -13.23442 galactic Cas Second-epoch detections are separated by 4.6" and 5.0 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 414658309087852416 | 00:46:04.57 +49:37:43.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:04.86 +49:37:41.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:04.86 +49:37:41.0: 13.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 04.86 +49 37 41.0 9.4 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 414658309087852416,2461231.6985,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414658309087852416 20260710.1985 9.38CV 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 10.1985 2461231.6985 9.56 00:34:22.76 +49:57:18.7
120.11939 -12.82338 galactic Cas Second-epoch detections are separated by 2.2" and 4.8 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 391491908326233088 | 00:34:22.58 +49:57:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=-0.007+/-0.028 (A)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:22.76 +49:57:18.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:22.76 +49:57:18.7: 13.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 22.76 +49 57 18.7 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 391491908326233088,2461231.6985,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391491908326233088 20260710.1985 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.52 00:34:03.66 +49:02:32.9
120.00204 -13.73040 galactic Cas Second-epoch detections are separated by 3.4" 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 | Gaia DR3 391347906663149312 | 00:34:03.37 +49:02:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:03.66 +49:02:32.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:03.66 +49:02:32.9: 13.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 03.66 +49 02 32.9 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
Gaia DR3 391347906663149312,2461231.6985,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391347906663149312 20260710.1985 9.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.41 00:29:53.01 +50:05:46.7
119.39242 -12.62725 galactic Cas Second-epoch detections are separated by 8.0" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391649138485880064 | 00:29:54.03 +50:05:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:53.01 +50:05:46.7: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:53.01 +50:05:46.7: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 29 53.01 +50 05 46.7 9.4 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 391649138485880064,2461231.6985,9.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391649138485880064 20260710.1985 9.41CV 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 10.1985 2461231.6985 9.59 00:31:51.19 +49:28:31.3
119.66540 -13.27213 galactic Cas Second-epoch detections are separated by 5.3" and 4.8 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 391572378834213376 | 00:31:51.00 +49:28:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.023+/-0.029 (A)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:51.19 +49:28:31.3: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:51.19 +49:28:31.3: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 31 51.19 +49 28 31.3 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 391572378834213376,2461231.6985,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391572378834213376 20260710.1985 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.50 00:33:18.41 +49:37:35.2
119.91855 -13.13919 galactic Cas Second-epoch detections are separated by 2.4" 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 | Large-amplitude variable Gaia DR2 391390340939844736 | 00:33:18.20 +49:37:37.4 (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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:18.41 +49:37:35.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:18.41 +49:37:35.2: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 33 18.41 +49 37 35.2 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
Large-amplitude variable Gaia DR2 391390340939844736,2461231.6985,9.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391390340939844736 20260710.1985 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 10.1985 2461231.6985 9.60 00:34:02.57 +49:31:15.8
120.03314 -13.25276 galactic Cas Second-epoch detections are separated by 1.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391385835515805568 | 00:34:02.38 +49:31:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:02.57 +49:31:15.8: 12.89 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:02.57 +49:31:15.8: 12.74 +/- 0.20 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 10.1985* 00 34 02.57 +49 31 15.8 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391385835515805568,2461231.6985,9.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391385835515805568 20260710.1985 9.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.52 00:29:36.60 +48:56:00.8
119.24381 -13.78182 galactic Cas Second-epoch detections are separated by 4.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391168170871414528 | 00:29:36.42 +48:55:59.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.108+/-0.027 (A)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:36.60 +48:56:00.8: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:36.60 +48:56:00.8: 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 10.1985* 00 29 36.60 +48 56 00.8 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
Gaia DR3 391168170871414528,2461231.6985,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391168170871414528 20260710.1985 9.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.54 00:34:08.69 +48:55:40.6
120.00800 -13.84560 galactic Cas Second-epoch detections are separated by 7.7" 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 | Gaia DR3 391341343953168896 | 00:34:08.46 +48:55:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:08.69 +48:55:40.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:08.69 +48:55:40.6: 13.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 08.69 +48 55 40.6 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
Gaia DR3 391341343953168896,2461231.6985,9.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391341343953168896 20260710.1985 9.54CV 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 10.1985 2461231.6985 9.59 00:34:56.95 +48:53:46.8
120.14161 -13.88606 galactic Cas Second-epoch detections are separated by 6.2" 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 | Gaia DR3 391334231487350016 | 00:34:56.76 +48:53:45.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.706+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:56.95 +48:53:46.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:56.95 +48:53:46.8: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 56.95 +48 53 46.8 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391334231487350016,2461231.6985,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391334231487350016 20260710.1985 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.53 00:43:58.21 +49:10:33.6
121.67593 -13.67754 galactic Cas Second-epoch detections are separated by 7.3" and 5.3 pix
The object was found in VSX13" Gaia DR3 414631336691943936
Type: ROT
# Max. Min./Amp. JD0 Period
14.390 G 14.410 G K
ATTENTION: measured mag 9.53 is 4.9 mag brighter than the VSX record maximum brightness 14.39 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:58.21 +49:10:33.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:58.21 +49:10:33.6: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 58.21 +49 10 33.6 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
Gaia DR3 414631336691943936,2461231.6985,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414631336691943936 20260710.1985 9.53CV 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 10.1985 2461231.6985 9.65 00:33:26.77 +49:19:04.2
119.91892 -13.44863 galactic Cas Second-epoch detections are separated by 3.7" and 5.0 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 391379410244728576 | 00:33:26.53 +49:19:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.071+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:26.77 +49:19:04.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:26.77 +49:19:04.2: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 33 26.77 +49 19 04.2 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391379410244728576,2461231.6985,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391379410244728576 20260710.1985 9.65CV 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 10.1985 2461231.6985 9.69 00:30:37.49 +49:15:38.7
119.44276 -13.46994 galactic Cas Second-epoch detections are separated by 2.8" and 5.0 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 391551213234585984 | 00:30:37.29 +49:15:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.789+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:37.49 +49:15:38.7: 13.26 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:37.49 +49:15:38.7: 13.25 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 10.1985* 00 30 37.49 +49 15 38.7 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391551213234585984,2461231.6985,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391551213234585984 20260710.1985 9.69CV 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 10.1985 2461231.6985 9.57 00:31:59.22 +49:09:55.8
119.66296 -13.58275 galactic Cas Second-epoch detections are separated by 2.5" and 5.1 pix
The object was found in VSX22" Gaia DR3 391538534491189888
Type: ROT
# Max. Min./Amp. JD0 Period
16.050 G 16.140 G 1.986410000000 K
ATTENTION: measured mag 9.57 is 6.5 mag brighter than the VSX record maximum brightness 16.05 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:59.22 +49:09:55.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:59.22 +49:09:55.8: 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 10.1985* 00 31 59.22 +49 09 55.8 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391538534491189888,2461231.6985,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391538534491189888 20260710.1985 9.57CV 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 10.1985 2461231.6985 9.66 00:33:05.91 +49:26:24.6
119.87002 -13.32252 galactic Cas Second-epoch detections are separated by 2.9" and 5.2 pix
The object was found in VSX20" Gaia DR3 391569114659123840
Type: ROT
# Max. Min./Amp. JD0 Period
14.820 G 14.870 G K
ATTENTION: measured mag 9.66 is 5.2 mag brighter than the VSX record maximum brightness 14.82 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:05.91 +49:26:24.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:05.91 +49:26:24.6: 13.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 33 05.91 +49 26 24.6 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391569114659123840,2461231.6985,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391569114659123840 20260710.1985 9.66CV 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 10.1985 2461231.6985 9.49 00:39:34.85 +48:54:30.4
120.92517 -13.91710 galactic Cas Second-epoch detections are separated by 5.2" 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 | Gaia DR3 390640023034538624 | 00:39:34.45 +48:54:33.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:34.85 +48:54:30.4: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:34.85 +48:54:30.4: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 34.85 +48 54 30.4 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
Gaia DR3 390640023034538624,2461231.6985,9.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390640023034538624 20260710.1985 9.49CV 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 10.1985 2461231.6985 9.68 00:30:09.72 +49:12:21.9
119.36062 -13.51808 galactic Cas Second-epoch detections are separated by 3.6" and 4.9 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 391178547514649856 | 00:30:09.58 +49:12:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.277+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:09.72 +49:12:21.9: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:09.72 +49:12:21.9: 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 10.1985* 00 30 09.72 +49 12 21.9 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391178547514649856,2461231.6985,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391178547514649856 20260710.1985 9.68CV 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 10.1985 2461231.6985 9.67 00:34:35.21 +49:51:37.2
120.14701 -12.92027 galactic Cas Second-epoch detections are separated by 2.2" 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 | Gaia DR3 391489606220164480 | 00:34:35.05 +49:51:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:35.21 +49:51:37.2: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:35.21 +49:51:37.2: 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 10.1985* 00 34 35.21 +49 51 37.2 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391489606220164480,2461231.6985,9.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391489606220164480 20260710.1985 9.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.74 00:47:47.57 +50:59:21.3
122.34577 -11.87835 galactic Cas Second-epoch detections are separated by 6.7" 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 | Gaia DR3 415211810112413184 | 00:47:47.33 +50:59:24.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:47.57 +50:59:21.3: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:47.57 +50:59:21.3: 13.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 47.57 +50 59 21.3 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415211810112413184,2461231.6985,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415211810112413184 20260710.1985 9.74CV 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 10.1985 2461231.6985 9.74 00:44:27.71 +50:58:49.6
121.80999 -11.87611 galactic Cas Second-epoch detections are separated by 2.9" and 5.0 pix
The object was found in VSX 3" Gaia DR3 415246955825412736
Type: ROT
# Max. Min./Amp. JD0 Period
11.100 G 11.140 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:27.71 +50:58:49.6: 12.28 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:27.71 +50:58:49.6: 12.09 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.19 +/- 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 10.1985* 00 44 27.71 +50 58 49.6 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415246955825412736,2461231.6985,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415246955825412736 20260710.1985 9.74CV 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 10.1985 2461231.6985 9.74 00:30:43.92 +49:15:29.0
119.46045 -13.47408 galactic Cas Second-epoch detections are separated by 3.0" and 5.0 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 391551041435899136 | 00:30:43.75 +49:15:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.313+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:43.92 +49:15:29.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:43.92 +49:15:29.0: 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 10.1985* 00 30 43.92 +49 15 29.0 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391551041435899136,2461231.6985,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391551041435899136 20260710.1985 9.74CV 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 10.1985 2461231.6985 9.78 00:33:00.64 +49:33:16.6
119.86402 -13.20734 galactic Cas Second-epoch detections are separated by 2.8" 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 | Gaia DR3 391575986603872768 | 00:33:00.39 +49:33:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:00.64 +49:33:16.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:00.64 +49:33:16.6: 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 10.1985* 00 33 00.64 +49 33 16.6 9.8 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 391575986603872768,2461231.6985,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391575986603872768 20260710.1985 9.78CV 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 10.1985 2461231.6985 9.76 00:42:56.93 +50:54:49.2
121.56446 -11.93554 galactic Cas Second-epoch detections are separated by 2.5" 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 | Gaia DR3 414874118304382080 | 00:42:56.03 +50:54:55.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:56.93 +50:54:49.2: 13.11 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:56.93 +50:54:49.2: 13.01 +/- 0.27 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 10.1985* 00 42 56.93 +50 54 49.2 9.8 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 414874118304382080,2461231.6985,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414874118304382080 20260710.1985 9.76CV 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 10.1985 2461231.6985 9.85 00:42:00.91 +50:58:01.7
121.41618 -11.87688 galactic Cas Second-epoch detections are separated by 2.4" and 4.9 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 414883846409015424 | 00:42:00.14 +50:58:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:00.91 +50:58:01.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:00.91 +50:58:01.7: 12.71 +/- 0.22 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 00.91 +50 58 01.7 9.8 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 414883846409015424,2461231.6985,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414883846409015424 20260710.1985 9.85CV 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 10.1985 2461231.6985 9.80 00:34:52.01 +49:01:28.4
120.13645 -13.75723 galactic Cas Second-epoch detections are separated by 4.2" and 5.0 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 391336877187154432 | 00:34:51.74 +49:01:28.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:52.01 +49:01:28.4: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:52.01 +49:01:28.4: 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 10.1985* 00 34 52.01 +49 01 28.4 9.8 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 391336877187154432,2461231.6985,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391336877187154432 20260710.1985 9.80CV 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 10.1985 2461231.6985 10.12 00:56:52.48 +57:23:42.3
123.66761 -5.46890 galactic Cas Second-epoch detections are separated by 6.9" and 4.8 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 J014.1842+57.3974 | 00:56:47.94 +57:23:58.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:56:52.48 +57:23:42.3: 12.52 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:56:52.48 +57:23:42.3: 12.12 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 10.1985* 00 56 52.48 +57 23 42.3 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
ATO J014.1842+57.3974,2461231.6985,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014.1842+57.3974 20260710.1985 10.12CV 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 10.1985 2461231.6985 9.91 00:35:17.56 +49:14:23.8
120.22245 -13.54685 galactic Cas Second-epoch detections are separated by 5.2" and 5.1 pix
The object was found in VSX 2" ASASSN-V J003517.47+491422.5
Type: L
# Max. Min./Amp. JD0 Period
11.940 V 12.020 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:17.56 +49:14:23.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:17.56 +49:14:23.8: 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 10.1985* 00 35 17.56 +49 14 23.8 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003517.47+491422.5,2461231.6985,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J003517.47+491422.5 20260710.1985 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.76 00:39:23.37 +48:58:48.7
120.89638 -13.84393 galactic Cas Second-epoch detections are separated by 5.0" and 5.1 pix
The object was found in VSX18" Gaia DR3 390640920686063360
Type: ROT
# Max. Min./Amp. JD0 Period
15.580 G 15.620 G F
ATTENTION: measured mag 9.76 is 5.8 mag brighter than the VSX record maximum brightness 15.58 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:23.37 +48:58:48.7: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:23.37 +48:58:48.7: 13.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 23.37 +48 58 48.7 9.8 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 390640920686063360,2461231.6985,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390640920686063360 20260710.1985 9.76CV 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 10.1985 2461231.6985 9.76 00:40:58.27 +48:54:05.6
121.16001 -13.93418 galactic Cas Second-epoch detections are separated by 6.3" 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 | Gaia DR3 390625660663901568 | 00:40:57.83 +48:54:05.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:58.27 +48:54:05.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:58.27 +48:54:05.6: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 40 58.27 +48 54 05.6 9.8 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 390625660663901568,2461231.6985,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390625660663901568 20260710.1985 9.76CV 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 10.1985 2461231.6985 9.94 00:34:16.96 +49:38:26.3
120.08143 -13.13614 galactic Cas Second-epoch detections are separated by 4.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391480844490558848 | 00:34:16.73 +49:38:29.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:16.96 +49:38:26.3: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:16.96 +49:38:26.3: 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 10.1985* 00 34 16.96 +49 38 26.3 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391480844490558848,2461231.6985,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391480844490558848 20260710.1985 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.87 00:39:42.16 +49:10:15.2
120.95845 -13.65589 galactic Cas Second-epoch detections are separated by 5.2" 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 | Gaia DR3 390649751135402752 | 00:39:41.81 +49:10:18.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:42.16 +49:10:15.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:42.16 +49:10:15.2: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 42.16 +49 10 15.2 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390649751135402752,2461231.6985,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390649751135402752 20260710.1985 9.87CV 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 10.1985 2461231.6985 9.96 00:32:20.07 +49:32:47.4
119.75106 -13.20723 galactic Cas Second-epoch detections are separated by 2.1" and 5.0 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 391573615787108736 | 00:32:19.92 +49:32:49.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.306+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:32:20.07 +49:32:47.4: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:32:20.07 +49:32:47.4: 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 10.1985* 00 32 20.07 +49 32 47.4 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391573615787108736,2461231.6985,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391573615787108736 20260710.1985 9.96CV 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 10.1985 2461231.6985 9.96 00:34:04.42 +49:01:31.6
120.00295 -13.74753 galactic Cas Second-epoch detections are separated by 4.8" and 5.0 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 391347872303419264 | 00:34:04.16 +49:01:31.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:04.42 +49:01:31.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:04.42 +49:01:31.6: 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 10.1985* 00 34 04.42 +49 01 31.6 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391347872303419264,2461231.6985,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391347872303419264 20260710.1985 9.96CV 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 10.1985 2461231.6985 10.09 00:47:24.18 +50:34:15.5
122.27623 -12.29564 galactic Cas Second-epoch detections are separated by 8.4" 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 | Large-amplitude variable Gaia DR2 415176453938645760 | 00:47:23.96 +50:34:20.5 (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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:24.18 +50:34:15.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:24.18 +50:34:15.5: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 24.18 +50 34 15.5 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 415176453938645760,2461231.6985,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415176453938645760 20260710.1985 10.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.07 00:34:36.11 +49:29:11.0
120.12374 -13.29354 galactic Cas Second-epoch detections are separated by 1.5" and 5.0 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 391385186979127296 | 00:34:35.93 +49:29:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:36.11 +49:29:11.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:36.11 +49:29:11.0: 13.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 36.11 +49 29 11.0 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391385186979127296,2461231.6985,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391385186979127296 20260710.1985 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.01 00:34:35.94 +49:33:31.0
120.12824 -13.22145 galactic Cas Second-epoch detections are separated by 0.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391479225284869376 | 00:34:36.11 +49:33:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.309+/-0.026 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:35.94 +49:33:31.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:35.94 +49:33:31.0: 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 10.1985* 00 34 35.94 +49 33 31.0 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391479225284869376,2461231.6985,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391479225284869376 20260710.1985 10.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.95 00:26:50.36 +49:10:19.8
118.80142 -13.50220 galactic Cas Second-epoch detections are separated by 0.6" and 5.1 pix
The object was found in VSX 3" Gaia DR3 391213216488083712
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.680 G 11.730 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:26:50.36 +49:10:19.8: 13.58 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:26:50.36 +49:10:19.8: 13.34 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.58 +/- 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 10.1985* 00 26 50.36 +49 10 19.8 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391213216488083712,2461231.6985,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391213216488083712 20260710.1985 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.02 00:47:01.14 +51:22:05.0
122.22812 -11.49765 galactic Cas Second-epoch detections are separated by 5.1" 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 | Gaia DR3 415227684311327616 | 00:47:00.53 +51:22:07.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:01.14 +51:22:05.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:01.14 +51:22:05.0: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 01.14 +51 22 05.0 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415227684311327616,2461231.6985,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415227684311327616 20260710.1985 10.02CV 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 10.1985 2461231.6985 10.06 00:32:52.96 +48:59:29.8
119.79990 -13.76726 galactic Cas Second-epoch detections are separated by 3.8" 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 | Large-amplitude variable Gaia DR2 391344711207263744 | 00:32:52.69 +48:59:29.3 (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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:32:52.96 +48:59:29.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:32:52.96 +48:59:29.8: 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 10.1985* 00 32 52.96 +48 59 29.8 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
Large-amplitude variable Gaia DR2 391344711207263744,2461231.6985,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391344711207263744 20260710.1985 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 10.1985 2461231.6985 9.98 00:27:32.28 +48:49:11.3
118.88374 -13.86400 galactic Cas Second-epoch detections are separated by 3.3" 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 | Gaia DR3 391198304358400512 | 00:27:32.06 +48:49:10.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.286+/-0.027 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:32.28 +48:49:11.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:32.28 +48:49:11.3: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 27 32.28 +48 49 11.3 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391198304358400512,2461231.6985,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391198304358400512 20260710.1985 9.98CV 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 10.1985 2461231.6985 10.01 00:38:16.91 +49:08:28.6
120.71815 -13.67391 galactic Cas Second-epoch detections are separated by 2.4" and 5.2 pix
The object was found in VSX 0" Gaia DR3 391396383955618688
Type: ROT
# Max. Min./Amp. JD0 Period
12.200 G 12.240 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:16.91 +49:08:28.6: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:16.91 +49:08:28.6: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 16.91 +49 08 28.6 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391396383955618688,2461231.6985,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391396383955618688 20260710.1985 10.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.15 00:39:11.60 +50:29:50.6
120.93927 -12.32698 galactic Cas Second-epoch detections are separated by 2.8" and 5.0 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 415506994623651840 | 00:39:13.86 +50:30:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:11.60 +50:29:50.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:11.60 +50:29:50.6: 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 10.1985* 00 39 11.60 +50 29 50.6 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415506994623651840,2461231.6985,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415506994623651840 20260710.1985 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.04 00:48:12.06 +50:51:51.2
122.40976 -12.00424 galactic Cas Second-epoch detections are separated by 7.6" 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 J012.0419+50.8550 | 00:48:11.79 +50:51:55.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:12.06 +50:51:51.2: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:12.06 +50:51:51.2: 13.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 48 12.06 +50 51 51.2 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J012.0419+50.8550,2461231.6985,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012.0419+50.8550 20260710.1985 10.04CV 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 10.1985 2461231.6985 9.96 00:43:16.28 +49:08:58.6
121.55756 -13.70034 galactic Cas Second-epoch detections are separated by 7.5" 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 | Gaia DR3 390613570334703360 | 00:43:15.95 +49:09:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:16.28 +49:08:58.6: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:16.28 +49:08:58.6: 13.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 16.28 +49 08 58.6 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390613570334703360,2461231.6985,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390613570334703360 20260710.1985 9.96CV 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 10.1985 2461231.6985 10.09 00:31:33.33 +49:18:21.9
119.60208 -13.43708 galactic Cas Second-epoch detections are separated by 8.0" and 4.8 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 391546299791997824 | 00:31:33.13 +49:18:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:33.33 +49:18:21.9: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:33.33 +49:18:21.9: 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 10.1985* 00 31 33.33 +49 18 21.9 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391546299791997824,2461231.6985,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391546299791997824 20260710.1985 10.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.97 00:34:49.24 +49:02:01.6
120.12930 -13.74752 galactic Cas Second-epoch detections are separated by 5.3" and 4.9 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 391336877187154432 | 00:34:51.74 +49:01:28.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:49.24 +49:02:01.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:49.24 +49:02:01.6: 13.14 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.14 +/- 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 10.1985* 00 34 49.24 +49 02 01.6 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391336877187154432,2461231.6985,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391336877187154432 20260710.1985 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.10 00:34:33.44 +49:23:40.3
120.10997 -13.38471 galactic Cas Second-epoch detections are separated by 1.3" and 5.0 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 391382777499092608 | 00:34:33.17 +49:23:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:33.44 +49:23:40.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:33.44 +49:23:40.3: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 33.44 +49 23 40.3 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391382777499092608,2461231.6985,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391382777499092608 20260710.1985 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.05 00:42:29.35 +50:06:33.1
121.46116 -12.73700 galactic Cas Second-epoch detections are separated by 0.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414733071577778944 | 00:42:29.24 +50:06:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.900+/-0.027 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:29.35 +50:06:33.1: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:29.35 +50:06:33.1: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 29.35 +50 06 33.1 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414733071577778944,2461231.6985,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414733071577778944 20260710.1985 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 9.96 00:46:53.59 +49:51:36.0
122.18021 -13.00512 galactic Cas Second-epoch detections are separated by 6.0" 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 | Gaia DR3 414568492729560320 | 00:46:53.28 +49:51:37.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:53.59 +49:51:36.0: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:53.59 +49:51:36.0: 13.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 53.59 +49 51 36.0 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414568492729560320,2461231.6985,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414568492729560320 20260710.1985 9.96CV 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 10.1985 2461231.6985 10.20 00:48:47.12 +51:11:36.0
122.50755 -11.67623 galactic Cas Second-epoch detections are separated by 2.4" 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 | Gaia DR3 415034440845266048 | 00:48:46.09 +51:11:43.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:47.12 +51:11:36.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:47.12 +51:11:36.0: 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 10.1985* 00 48 47.12 +51 11 36.0 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415034440845266048,2461231.6985,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415034440845266048 20260710.1985 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.12 00:34:43.02 +49:42:52.9
120.15853 -13.06699 galactic Cas Second-epoch detections are separated by 1.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391482081443505280 | 00:34:42.89 +49:42:53.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.834+/-0.032 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:43.02 +49:42:52.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:43.02 +49:42:52.9: 13.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 43.02 +49 42 52.9 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391482081443505280,2461231.6985,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391482081443505280 20260710.1985 10.12CV 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 10.1985 2461231.6985 10.12 00:29:55.57 +49:08:55.6
119.31609 -13.57188 galactic Cas Second-epoch detections are separated by 4.9" and 4.8 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 J007.4798+49.1549 | 00:29:55.43 +49:08:56.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.065+/-0.029 (A)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:55.57 +49:08:55.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:55.57 +49:08:55.6: 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 10.1985* 00 29 55.57 +49 08 55.6 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J007.4798+49.1549,2461231.6985,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J007.4798+49.1549 20260710.1985 10.12CV 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 10.1985 2461231.6985 10.27 00:46:18.32 +50:52:22.2
122.10418 -11.99067 galactic Cas Second-epoch detections are separated by 4.4" 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 | ATO J011.5756+50.8833 | 00:46:18.20 +50:52:21.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.247+/-0.026 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:18.32 +50:52:22.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:18.32 +50:52:22.2: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 18.32 +50 52 22.2 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J011.5756+50.8833,2461231.6985,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.5756+50.8833 20260710.1985 10.27CV 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 10.1985 2461231.6985 10.19 00:45:52.74 +50:50:45.3
122.03482 -12.01615 galactic Cas Second-epoch detections are separated by 5.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J011.4637+50.8503 | 00:45:52.61 +50:50:49.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:52.74 +50:50:45.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:52.74 +50:50:45.3: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 52.74 +50 50 45.3 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J011.4637+50.8503,2461231.6985,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.4637+50.8503 20260710.1985 10.19CV 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 10.1985 2461231.6985 10.18 00:41:44.34 +49:24:11.3
121.30992 -13.43806 galactic Cas Second-epoch detections are separated by 4.2" and 4.7 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 390668717714476160 | 00:41:42.71 +49:23:37.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:44.34 +49:24:11.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:44.34 +49:24:11.3: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 44.34 +49 24 11.3 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390668717714476160,2461231.6985,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390668717714476160 20260710.1985 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.31 00:43:57.38 +51:14:00.1
121.73639 -11.62102 galactic Cas Second-epoch detections are separated by 2.0" and 5.3 pix
The object was found in VSX18" T-Cas0-05165
Type: EA
# Max. Min./Amp. JD0 Period
12.180 R Y 0.064 R 2453277.98700 2.358650000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:57.38 +51:14:00.1: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:57.38 +51:14:00.1: 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 10.1985* 00 43 57.38 +51 14 00.1 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
T-Cas0-05165,2461231.6985,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
T-Cas0-05165 20260710.1985 10.31CV 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 10.1985 2461231.6985 10.21 00:30:57.89 +49:16:02.0
119.50015 -13.46806 galactic Cas Second-epoch detections are separated by 3.9" and 4.9 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 391551831709883008 | 00:30:57.72 +49:16:02.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=10.502+/- (unrealisitic color!)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:57.89 +49:16:02.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:57.89 +49:16:02.0: 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 10.1985* 00 30 57.89 +49 16 02.0 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391551831709883008,2461231.6985,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391551831709883008 20260710.1985 10.21CV 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 10.1985 2461231.6985 10.12 00:39:33.86 +49:10:19.8
120.93527 -13.65355 galactic Cas Second-epoch detections are separated by 4.2" and 5.2 pix
The object was found in VSX21" Gaia DR3 390649716779198848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.660 G 13.690 G F
ATTENTION: measured mag 10.12 is 3.5 mag brighter than the VSX record maximum brightness 13.66 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:33.86 +49:10:19.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:33.86 +49:10:19.8: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 33.86 +49 10 19.8 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390649716779198848,2461231.6985,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390649716779198848 20260710.1985 10.12CV 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 10.1985 2461231.6985 10.18 00:47:37.20 +50:24:26.3
122.30895 -12.45982 galactic Cas Second-epoch detections are separated by 4.2" 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 | Gaia DR3 414611992158362624 | 00:47:36.93 +50:24:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:37.20 +50:24:26.3: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:37.20 +50:24:26.3: 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 10.1985* 00 47 37.20 +50 24 26.3 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414611992158362624,2461231.6985,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414611992158362624 20260710.1985 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.10 00:44:43.93 +49:42:46.0
121.81882 -13.14448 galactic Cas Second-epoch detections are separated by 5.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414668582648149760 | 00:44:43.58 +49:42:48.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:43.93 +49:42:46.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:43.93 +49:42:46.0: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 43.93 +49 42 46.0 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414668582648149760,2461231.6985,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414668582648149760 20260710.1985 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.32 00:46:47.03 +51:14:07.0
122.18817 -11.62975 galactic Cas Second-epoch detections are separated by 5.9" 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 | ATO J011.7004+51.2346 | 00:46:46.54 +51:14:12.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:47.03 +51:14:07.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:47.03 +51:14:07.0: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 47.03 +51 14 07.0 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J011.7004+51.2346,2461231.6985,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.7004+51.2346 20260710.1985 10.32CV 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 10.1985 2461231.6985 10.26 00:46:38.70 +50:41:13.3
122.15533 -12.17749 galactic Cas Second-epoch detections are separated by 4.9" and 4.8 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 415180955067461504 | 00:46:38.50 +50:41:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:38.70 +50:41:13.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:38.70 +50:41:13.3: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 38.70 +50 41 13.3 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415180955067461504,2461231.6985,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415180955067461504 20260710.1985 10.26CV 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 10.1985 2461231.6985 10.22 00:45:35.72 +50:31:49.7
121.98157 -12.33050 galactic Cas Second-epoch detections are separated by 4.6" and 5.0 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 414815264371669120 | 00:45:35.56 +50:31:48.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.823+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:35.72 +50:31:49.7: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:35.72 +50:31:49.7: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 35.72 +50 31 49.7 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414815264371669120,2461231.6985,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414815264371669120 20260710.1985 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.29 00:47:41.69 +50:47:29.4
122.32700 -12.07585 galactic Cas Second-epoch detections are separated by 6.9" and 4.9 pix
The object was found in VSX 5" Gaia DR3 415185387470501376
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.560 G 11.650 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:41.69 +50:47:29.4: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:41.69 +50:47:29.4: 13.18 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 41.69 +50 47 29.4 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415185387470501376,2461231.6985,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415185387470501376 20260710.1985 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.19 00:36:30.32 +49:32:05.3
120.44373 -13.26479 galactic Cas Second-epoch detections are separated by 1.0" 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 | Gaia DR3 391470261691517440 | 00:36:30.23 +49:32:06.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.192+/-0.027 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:30.32 +49:32:05.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:30.32 +49:32:05.3: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 30.32 +49 32 05.3 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391470261691517440,2461231.6985,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391470261691517440 20260710.1985 10.19CV 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 10.1985 2461231.6985 10.10 00:38:19.01 +49:03:44.9
120.71978 -13.75291 galactic Cas Second-epoch detections are separated by 3.5" 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 | ATO J009.5780+49.0628 | 00:38:18.75 +49:03:46.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:19.01 +49:03:44.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:19.01 +49:03:44.9: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 19.01 +49 03 44.9 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
ATO J009.5780+49.0628,2461231.6985,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.5780+49.0628 20260710.1985 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.29 00:33:07.73 +49:00:57.2
119.84319 -13.74602 galactic Cas Second-epoch detections are separated by 6.1" and 4.9 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 J008.2810+49.0145 | 00:33:07.45 +49:00:52.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:07.73 +49:00:57.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:07.73 +49:00:57.2: 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 10.1985* 00 33 07.73 +49 00 57.2 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.2810+49.0145,2461231.6985,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.2810+49.0145 20260710.1985 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.23 00:42:49.44 +50:06:14.3
121.51599 -12.74409 galactic Cas Second-epoch detections are separated by 1.9" and 5.0 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 J010.7166+50.0963 | 00:42:49.41 +50:06:14.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.052+/-0.027 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:49.44 +50:06:14.3: 12.15 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:49.44 +50:06:14.3: 12.17 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 49.44 +50 06 14.3 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.7166+50.0963,2461231.6985,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.7166+50.0963 20260710.1985 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.36 00:29:41.61 +48:41:39.6
119.23647 -14.02133 galactic Cas Second-epoch detections are separated by 6.0" and 4.9 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 391141400336403584 | 00:29:41.37 +48:41:39.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.137+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:41.61 +48:41:39.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:41.61 +48:41:39.6: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 29 41.61 +48 41 39.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391141400336403584,2461231.6985,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391141400336403584 20260710.1985 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.12 00:37:06.77 +48:54:59.7
120.50845 -13.88775 galactic Cas Second-epoch detections are separated by 2.0" 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 391306503178706048 | 00:37:06.38 +48:54:59.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:06.77 +48:54:59.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:06.77 +48:54:59.7: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 37 06.77 +48 54 59.7 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391306503178706048,2461231.6985,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391306503178706048 20260710.1985 10.12CV 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 10.1985 2461231.6985 10.20 00:42:34.61 +50:13:17.7
121.47963 -12.62518 galactic Cas Second-epoch detections are separated by 4.1" and 4.8 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 414734656426309632 | 00:42:37.54 +50:13:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.308+/-0.026 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:34.61 +50:13:17.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:34.61 +50:13:17.7: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 34.61 +50 13 17.7 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414734656426309632,2461231.6985,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414734656426309632 20260710.1985 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.26 00:39:17.09 +49:07:03.5
120.88558 -13.70582 galactic Cas Second-epoch detections are separated by 7.4" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391393914353044864 | 00:39:16.84 +49:07:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:17.09 +49:07:03.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:17.09 +49:07:03.5: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 17.09 +49 07 03.5 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391393914353044864,2461231.6985,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391393914353044864 20260710.1985 10.26CV 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 10.1985 2461231.6985 10.30 00:35:23.59 +49:04:22.7
120.22829 -13.71453 galactic Cas Second-epoch detections are separated by 4.0" 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 | ATO J008.8563+49.0712 | 00:35:23.43 +49:04:22.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.560+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:23.59 +49:04:22.7: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:23.59 +49:04:22.7: 13.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 23.59 +49 04 22.7 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.8563+49.0712,2461231.6985,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.8563+49.0712 20260710.1985 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.32 00:35:46.59 +49:23:09.7
120.31291 -13.40606 galactic Cas Second-epoch detections are separated by 0.7" and 5.0 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 J008.9313+49.3830 | 00:35:46.42 +49:23:13.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:46.59 +49:23:09.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:46.59 +49:23:09.7: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 46.59 +49 23 09.7 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.9313+49.3830,2461231.6985,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.9313+49.3830 20260710.1985 10.32CV 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 10.1985 2461231.6985 10.14 00:39:01.48 +49:30:16.9
120.86154 -13.31715 galactic Cas Second-epoch detections are separated by 2.5" and 4.8 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 391429785919972992 | 00:39:01.29 +49:30:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:01.48 +49:30:16.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:01.48 +49:30:16.9: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 01.48 +49 30 16.9 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391429785919972992,2461231.6985,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391429785919972992 20260710.1985 10.14CV 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 10.1985 2461231.6985 10.33 00:48:11.86 +50:59:22.9
122.41087 -11.87878 galactic Cas Second-epoch detections are separated by 8.4" 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 | Gaia DR3 415025442890741248 | 00:48:14.47 +50:59:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:11.86 +50:59:22.9: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:11.86 +50:59:22.9: 13.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 48 11.86 +50 59 22.9 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415025442890741248,2461231.6985,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415025442890741248 20260710.1985 10.33CV 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 10.1985 2461231.6985 10.23 00:36:24.00 +49:29:18.0
120.42334 -13.31015 galactic Cas Second-epoch detections are separated by 1.6" 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 | ATO J009.0999+49.4885 | 00:36:23.99 +49:29:18.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.100+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:24.00 +49:29:18.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:24.00 +49:29:18.0: 13.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 24.00 +49 29 18.0 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J009.0999+49.4885,2461231.6985,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.0999+49.4885 20260710.1985 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.22 00:38:30.74 +49:12:54.0
120.76082 -13.60225 galactic Cas Second-epoch detections are separated by 2.8" and 5.1 pix
The object was found in VSX 5" Gaia DR3 391398514258621568
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.490 G 11.540 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:30.74 +49:12:54.0: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:30.74 +49:12:54.0: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 30.74 +49 12 54.0 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391398514258621568,2461231.6985,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391398514258621568 20260710.1985 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.41 00:33:51.13 +49:19:04.6
119.98679 -13.45322 galactic Cas Second-epoch detections are separated by 4.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391379964298942848 | 00:33:50.86 +49:19:05.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:51.13 +49:19:04.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:51.13 +49:19:04.6: 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 10.1985* 00 33 51.13 +49 19 04.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391379964298942848,2461231.6985,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391379964298942848 20260710.1985 10.41CV 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 10.1985 2461231.6985 10.32 00:35:46.91 +49:26:55.0
120.31782 -13.34366 galactic Cas Second-epoch detections are separated by 1.0" 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 | Gaia DR3 391463252304917888 | 00:35:46.77 +49:26:56.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.278+/-0.026 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:46.91 +49:26:55.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:46.91 +49:26:55.0: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 46.91 +49 26 55.0 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391463252304917888,2461231.6985,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391463252304917888 20260710.1985 10.32CV 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 10.1985 2461231.6985 10.40 00:30:09.45 +49:34:50.7
119.39252 -13.14470 galactic Cas Second-epoch detections are separated by 2.7" and 4.8 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 391565846184775808 | 00:30:09.36 +49:34:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.185+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:09.45 +49:34:50.7: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:09.45 +49:34:50.7: 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 10.1985* 00 30 09.45 +49 34 50.7 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391565846184775808,2461231.6985,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391565846184775808 20260710.1985 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.40 00:39:37.63 +49:24:22.0
120.95717 -13.42035 galactic Cas Second-epoch detections are separated by 3.4" 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 | Gaia DR3 391426830982488320 | 00:39:37.38 +49:24:23.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:37.63 +49:24:22.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:37.63 +49:24:22.0: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 37.63 +49 24 22.0 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391426830982488320,2461231.6985,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391426830982488320 20260710.1985 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.30 00:42:54.09 +50:11:16.8
121.53165 -12.66054 galactic Cas Second-epoch detections are separated by 3.2" 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 | Gaia DR3 414734312827410560 | 00:42:54.01 +50:11:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:54.09 +50:11:16.8: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:54.09 +50:11:16.8: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 54.09 +50 11 16.8 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414734312827410560,2461231.6985,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414734312827410560 20260710.1985 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.29 00:36:35.64 +49:09:00.6
120.43505 -13.64960 galactic Cas Second-epoch detections are separated by 3.7" and 5.2 pix
The object was found in VSX12" Gaia DR3 391317979331254144
Type: S
# Max. Min./Amp. JD0 Period
17.540 G 18.520 G
ATTENTION: measured mag 10.29 is 7.2 mag brighter than the VSX record maximum brightness 17.54 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:35.64 +49:09:00.6: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:35.64 +49:09:00.6: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 35.64 +49 09 00.6 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391317979331254144,2461231.6985,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391317979331254144 20260710.1985 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.43 00:43:05.25 +51:03:48.0
121.59185 -11.78669 galactic Cas Second-epoch detections are separated by 5.1" 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 | Gaia DR3 415251804847489792 | 00:43:04.57 +51:03:53.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:05.25 +51:03:48.0: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:05.25 +51:03:48.0: 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 10.1985* 00 43 05.25 +51 03 48.0 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415251804847489792,2461231.6985,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415251804847489792 20260710.1985 10.43CV 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 10.1985 2461231.6985 10.35 00:47:50.76 +51:30:48.7
122.36194 -11.35425 galactic Cas Second-epoch detections are separated by 2.4" and 5.0 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 | Large-amplitude variable Gaia DR2 415323479258531712 | 00:47:50.68 +51:30:50.7 (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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:50.76 +51:30:48.7: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:50.76 +51:30:48.7: 13.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 50.76 +51 30 48.7 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 415323479258531712,2461231.6985,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415323479258531712 20260710.1985 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.39 00:44:29.36 +50:13:55.6
121.79327 -12.62427 galactic Cas Second-epoch detections are separated by 1.9" and 5.2 pix
The object was found in VSX16" Gaia DR3 414784478046217216
Type: ROT
# Max. Min./Amp. JD0 Period
15.950 G 15.960 G 0.721020000000 F
ATTENTION: measured mag 10.39 is 5.6 mag brighter than the VSX record maximum brightness 15.95 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:29.36 +50:13:55.6: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:29.36 +50:13:55.6: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 29.36 +50 13 55.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414784478046217216,2461231.6985,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414784478046217216 20260710.1985 10.39CV 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 10.1985 2461231.6985 10.36 00:34:40.93 +49:36:47.7
120.14581 -13.16783 galactic Cas Second-epoch detections are separated by 0.5" 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 | ATO J008.6760+49.6109 | 00:34:40.80 +49:36:50.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:40.93 +49:36:47.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:40.93 +49:36:47.7: 13.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 40.93 +49 36 47.7 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.6760+49.6109,2461231.6985,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.6760+49.6109 20260710.1985 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.40 00:34:23.47 +49:51:01.4
120.11404 -12.92807 galactic Cas Second-epoch detections are separated by 2.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 391489743662740992 | 00:34:23.23 +49:51:03.0 (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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:23.47 +49:51:01.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:23.47 +49:51:01.4: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 23.47 +49 51 01.4 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 391489743662740992,2461231.6985,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391489743662740992 20260710.1985 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.31 00:40:24.89 +49:16:21.4
121.08272 -13.55956 galactic Cas Second-epoch detections are separated by 1.5" and 5.0 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 390674627589497216 | 00:40:24.73 +49:16:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.558+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:24.89 +49:16:21.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:24.89 +49:16:21.4: 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 10.1985* 00 40 24.89 +49 16 21.4 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390674627589497216,2461231.6985,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390674627589497216 20260710.1985 10.31CV 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 10.1985 2461231.6985 10.29 00:45:44.72 +49:39:24.3
121.98566 -13.20454 galactic Cas Second-epoch detections are separated by 7.0" and 4.7 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 414661195304686464 | 00:45:44.45 +49:39:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:44.72 +49:39:24.3: 12.80 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:44.72 +49:39:24.3: 12.09 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.33 +/- 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 10.1985* 00 45 44.72 +49 39 24.3 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414661195304686464,2461231.6985,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414661195304686464 20260710.1985 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.34 00:33:46.17 +49:46:08.2
120.00559 -13.00239 galactic Cas Second-epoch detections are separated by 1.7" and 5.0 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 J008.4418+49.7694 | 00:33:46.05 +49:46:09.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.269+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:46.17 +49:46:08.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:46.17 +49:46:08.2: 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 10.1985* 00 33 46.17 +49 46 08.2 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.4418+49.7694,2461231.6985,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.4418+49.7694 20260710.1985 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.39 00:39:17.65 +49:05:13.0
120.88562 -13.73655 galactic Cas Second-epoch detections are separated by 3.8" 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 | Gaia DR3 391393776914096512 | 00:39:17.27 +49:05:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:17.65 +49:05:13.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:17.65 +49:05:13.0: 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 10.1985* 00 39 17.65 +49 05 13.0 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391393776914096512,2461231.6985,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391393776914096512 20260710.1985 10.39CV 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 10.1985 2461231.6985 10.95 23:38:10.97 +52:49:00.8
111.86242 -8.47324 galactic Cas Second-epoch detections are separated by 0.8" and 4.6 pix
The object was found in VSX 2" ZTF J233810.95+524903.0
Type: SR
# Max. Min./Amp. JD0 Period
12.653 r Y 0.375 r 2458343.79690 70.192939000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:38:10.97 +52:49:00.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:38:10.97 +52:49:00.8: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 23 38 10.97 +52 49 00.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J233810.95+524903.0,2461231.6985,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J233810.95+524903.0 20260710.1985 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.40 00:34:24.15 +49:22:46.1
120.08308 -13.39802 galactic Cas Second-epoch detections are separated by 5.1" and 4.8 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 391382644358520832 | 00:34:23.87 +49:22:46.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:24.15 +49:22:46.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:24.15 +49:22:46.1: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 24.15 +49 22 46.1 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391382644358520832,2461231.6985,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391382644358520832 20260710.1985 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.39 00:35:22.91 +49:49:47.5
120.27619 -12.95908 galactic Cas Second-epoch detections are separated by 2.5" and 4.8 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 391478473669308544 | 00:35:22.69 +49:49:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:22.91 +49:49:47.5: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:22.91 +49:49:47.5: 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 10.1985* 00 35 22.91 +49 49 47.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391478473669308544,2461231.6985,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391478473669308544 20260710.1985 10.39CV 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 10.1985 2461231.6985 10.43 00:30:52.73 +49:19:20.6
119.49042 -13.41193 galactic Cas Second-epoch detections are separated by 3.5" and 4.9 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 391552755124475264 | 00:30:52.67 +49:19:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.771+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:52.73 +49:19:20.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:52.73 +49:19:20.6: 13.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 30 52.73 +49 19 20.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391552755124475264,2461231.6985,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391552755124475264 20260710.1985 10.43CV 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 10.1985 2461231.6985 10.46 00:47:14.56 +50:21:14.0
122.24647 -12.51228 galactic Cas Second-epoch detections are separated by 5.8" and 4.9 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 414797981423661440 | 00:47:14.36 +50:21:15.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.696+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:14.56 +50:21:14.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:14.56 +50:21:14.0: 13.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 14.56 +50 21 14.0 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414797981423661440,2461231.6985,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414797981423661440 20260710.1985 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.36 00:45:21.83 +50:47:05.3
121.95020 -12.07536 galactic Cas Second-epoch detections are separated by 4.3" and 5.1 pix
The object was found in VSX 4" Gaia DR3 415194660304697088
Type: ROT
# Max. Min./Amp. JD0 Period
11.660 G 11.720 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:21.83 +50:47:05.3: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:21.83 +50:47:05.3: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 21.83 +50 47 05.3 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415194660304697088,2461231.6985,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415194660304697088 20260710.1985 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.28 00:38:25.76 +49:06:31.7
120.74121 -13.70760 galactic Cas Second-epoch detections are separated by 1.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391396010297080832 | 00:38:25.46 +49:06:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:25.76 +49:06:31.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:25.76 +49:06:31.7: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 25.76 +49 06 31.7 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391396010297080832,2461231.6985,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391396010297080832 20260710.1985 10.28CV 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 10.1985 2461231.6985 10.39 00:45:52.36 +50:24:02.4
122.02373 -12.46127 galactic Cas Second-epoch detections are separated by 3.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J011.4641+50.4023 | 00:45:52.17 +50:24:05.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:52.36 +50:24:02.4: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:52.36 +50:24:02.4: 13.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 52.36 +50 24 02.4 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J011.4641+50.4023,2461231.6985,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.4641+50.4023 20260710.1985 10.39CV 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 10.1985 2461231.6985 10.47 00:29:26.24 +49:15:18.3
119.24376 -13.45905 galactic Cas Second-epoch detections are separated by 4.3" and 4.9 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 391226303249926016 | 00:29:26.10 +49:15:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.291+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:26.24 +49:15:18.3: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:26.24 +49:15:18.3: 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 10.1985* 00 29 26.24 +49 15 18.3 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391226303249926016,2461231.6985,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391226303249926016 20260710.1985 10.47CV 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 10.1985 2461231.6985 10.36 00:46:46.22 +49:46:26.9
122.15826 -13.09060 galactic Cas Second-epoch detections are separated by 5.7" and 5.0 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 414753966598759424 | 00:46:46.07 +49:46:29.0 (Gaia DR3) | ROT (local) | 1.388740000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.646+/-0.023 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:46.22 +49:46:26.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:46.22 +49:46:26.9: 13.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 46.22 +49 46 26.9 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414753966598759424,2461231.6985,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414753966598759424 20260710.1985 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.42 00:41:06.82 +49:38:11.5
121.21529 -13.20081 galactic Cas Second-epoch detections are separated by 4.4" and 4.6 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 J010.2607+49.6434 | 00:41:06.88 +49:38:18.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:06.82 +49:38:11.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:06.82 +49:38:11.5: 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 10.1985* 00 41 06.82 +49 38 11.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.2607+49.6434,2461231.6985,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.2607+49.6434 20260710.1985 10.42CV 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 10.1985 2461231.6985 10.91 00:25:46.33 +57:59:01.6
119.52374 -4.71803 galactic Cas Second-epoch detections are separated by 1.3" and 4.7 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 421927382318018560 | 00:25:45.97 +57:59:06.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:25:46.33 +57:59:01.6: 13.19 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:25:46.33 +57:59:01.6: 13.08 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.14 +/- 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 10.1985* 00 25 46.33 +57 59 01.6 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 421927382318018560,2461231.6985,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 421927382318018560 20260710.1985 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.42 00:40:46.97 +50:18:52.3
121.18982 -12.52118 galactic Cas Second-epoch detections are separated by 4.8" and 4.8 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 414750908580993408 | 00:40:47.00 +50:18:56.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:46.97 +50:18:52.3: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:46.97 +50:18:52.3: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 40 46.97 +50 18 52.3 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414750908580993408,2461231.6985,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414750908580993408 20260710.1985 10.42CV 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 10.1985 2461231.6985 10.53 00:47:53.87 +51:24:28.5
122.36865 -11.45996 galactic Cas Second-epoch detections are separated by 5.5" and 4.7 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 J011.9675+51.4091 | 00:47:53.22 +51:24:32.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:53.87 +51:24:28.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:53.87 +51:24:28.5: 13.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 53.87 +51 24 28.5 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 J011.9675+51.4091,2461231.6985,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.9675+51.4091 20260710.1985 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 10.1985 2461231.6985 10.40 00:39:00.38 +49:13:32.7
120.84426 -13.59560 galactic Cas Second-epoch detections are separated by 3.2" 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 | Gaia DR3 391401095538341120 | 00:39:00.07 +49:13:36.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:00.38 +49:13:32.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:00.38 +49:13:32.7: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 00.38 +49 13 32.7 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391401095538341120,2461231.6985,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391401095538341120 20260710.1985 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.46 00:38:51.17 +49:35:21.5
120.83728 -13.23125 galactic Cas Second-epoch detections are separated by 3.0" and 4.8 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 391433565490957312 | 00:38:50.95 +49:35:24.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:51.17 +49:35:21.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:51.17 +49:35:21.5: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 51.17 +49 35 21.5 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391433565490957312,2461231.6985,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391433565490957312 20260710.1985 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.28 00:44:05.27 +49:44:08.0
121.71259 -13.11879 galactic Cas Second-epoch detections are separated by 4.9" 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 | Gaia DR3 414672121701447296 | 00:44:05.00 +49:44:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:05.27 +49:44:08.0: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:05.27 +49:44:08.0: 13.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 05.27 +49 44 08.0 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414672121701447296,2461231.6985,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414672121701447296 20260710.1985 10.28CV 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 10.1985 2461231.6985 10.34 00:38:26.79 +48:56:46.1
120.73540 -13.87020 galactic Cas Second-epoch detections are separated by 2.8" 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 | ATO J009.6098+48.9465 | 00:38:26.37 +48:56:47.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:26.79 +48:56:46.1: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:26.79 +48:56:46.1: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 26.79 +48 56 46.1 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J009.6098+48.9465,2461231.6985,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.6098+48.9465 20260710.1985 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.45 00:42:11.50 +50:45:53.0
121.43697 -12.08019 galactic Cas Second-epoch detections are separated by 2.6" 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 J010.5572+50.7645 | 00:42:11.46 +50:45:55.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.302+/-0.027 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:11.50 +50:45:53.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:11.50 +50:45:53.0: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 11.50 +50 45 53.0 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.5572+50.7645,2461231.6985,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.5572+50.7645 20260710.1985 10.45CV 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 10.1985 2461231.6985 10.48 00:38:58.05 +50:19:33.2
120.89385 -12.49651 galactic Cas Second-epoch detections are separated by 3.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J009.7502+50.3235 | 00:38:58.06 +50:19:32.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.027 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:58.05 +50:19:33.2: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:58.05 +50:19:33.2: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 58.05 +50 19 33.2 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 J009.7502+50.3235,2461231.6985,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.7502+50.3235 20260710.1985 10.48CV 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 10.1985 2461231.6985 10.59 00:48:01.29 +53:47:45.1
122.42105 -9.07250 galactic Cas Second-epoch detections are separated by 1.2" and 4.9 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 417072630462986880 | 00:48:02.78 +53:47:04.0 (Gaia DR3) | DSCT/GDOR (local) | 0.075834100000 (local) | Gaia3var=VARIABLE SpType: A7 1927AnHar.100...33C HD 232276
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:01.29 +53:47:45.1: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:01.29 +53:47:45.1: 13.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 48 01.29 +53 47 45.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 417072630462986880,2461231.6985,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 417072630462986880 20260710.1985 10.59CV 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 10.1985 2461231.6985 10.40 00:44:58.37 +50:03:21.4
121.86783 -12.80245 galactic Cas Second-epoch detections are separated by 2.5" 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 | Gaia DR3 414773551649515136 | 00:44:58.12 +50:03:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.390+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:58.37 +50:03:21.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:58.37 +50:03:21.4: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 58.37 +50 03 21.4 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414773551649515136,2461231.6985,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414773551649515136 20260710.1985 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.16 23:23:16.71 +52:26:44.9
109.57367 -8.12443 galactic And Second-epoch detections are separated by 1.6" and 4.6 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 J350.8041+52.4529 | 23:23:13.95 +52:26:43.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.699+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:23:16.71 +52:26:44.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:23:16.71 +52:26:44.9: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 23 23 16.71 +52 26 44.9 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.8041+52.4529,2461231.6985,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J350.8041+52.4529 20260710.1985 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.44 00:46:51.47 +50:27:44.6
122.18563 -12.40272 galactic Cas Second-epoch detections are separated by 4.0" 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 | ATO J011.6995+50.4563 | 00:46:51.18 +50:27:44.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:51.47 +50:27:44.6: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:51.47 +50:27:44.6: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 51.47 +50 27 44.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J011.6995+50.4563,2461231.6985,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.6995+50.4563 20260710.1985 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.46 00:37:19.86 +49:22:16.7
120.57167 -13.43578 galactic Cas Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 391412812206002560 | 00:37:19.69 +49:22:18.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:19.86 +49:22:16.7: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:19.86 +49:22:16.7: 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 10.1985* 00 37 19.86 +49 22 16.7 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
Large-amplitude variable Gaia DR2 391412812206002560,2461231.6985,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391412812206002560 20260710.1985 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.54 00:45:46.68 +50:38:15.2
122.01374 -12.22410 galactic Cas Second-epoch detections are separated by 3.1" 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 | Gaia DR3 414817562175256192 | 00:45:46.53 +50:38:14.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.397+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:46.68 +50:38:15.2: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:46.68 +50:38:15.2: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 46.68 +50 38 15.2 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414817562175256192,2461231.6985,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414817562175256192 20260710.1985 10.54CV 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 10.1985 2461231.6985 10.50 00:35:36.16 +49:54:16.9
120.31750 -12.88665 galactic Cas Second-epoch detections are separated by 2.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 391501803927717120 | 00:35:35.96 +49:54:17.2 (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) J-Ks=0.420+/-0.027 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:36.16 +49:54:16.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:36.16 +49:54:16.9: 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 10.1985* 00 35 36.16 +49 54 16.9 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
Large-amplitude variable Gaia DR2 391501803927717120,2461231.6985,10.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391501803927717120 20260710.1985 10.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.40 00:38:59.19 +49:06:42.7
120.83510 -13.70919 galactic Cas Second-epoch detections are separated by 3.5" 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 | Gaia DR3 391394429749118720 | 00:38:58.93 +49:06:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:59.19 +49:06:42.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:59.19 +49:06:42.7: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 59.19 +49 06 42.7 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391394429749118720,2461231.6985,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391394429749118720 20260710.1985 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.52 00:45:42.35 +51:05:26.9
122.01258 -11.77071 galactic Cas Second-epoch detections are separated by 8.4" and 4.9 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 415205762798371200 | 00:45:41.68 +51:05:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:42.35 +51:05:26.9: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:42.35 +51:05:26.9: 13.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 42.35 +51 05 26.9 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415205762798371200,2461231.6985,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415205762798371200 20260710.1985 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.61 00:41:21.50 +51:05:37.9
121.31576 -11.74626 galactic Cas Second-epoch detections are separated by 3.6" and 4.9 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 415641925317110400 | 00:41:21.22 +51:05:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:21.50 +51:05:37.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:21.50 +51:05:37.9: 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 10.1985* 00 41 21.50 +51 05 37.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415641925317110400,2461231.6985,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415641925317110400 20260710.1985 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.52 00:36:47.78 +49:20:39.3
120.48071 -13.45780 galactic Cas Second-epoch detections are separated by 3.7" and 4.8 pix
The object was found in VSX 4" Gaia DR3 391413980440161536
Type: ROT
# Max. Min./Amp. JD0 Period
11.820 G 11.880 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:47.78 +49:20:39.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:47.78 +49:20:39.3: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 47.78 +49 20 39.3 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391413980440161536,2461231.6985,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391413980440161536 20260710.1985 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.46 00:48:36.44 +51:29:37.3
122.48251 -11.37558 galactic Cas Second-epoch detections are separated by 1.4" and 5.0 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 415325334687634944 | 00:48:36.26 +51:29:39.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:36.44 +51:29:37.3: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:36.44 +51:29:37.3: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 48 36.44 +51 29 37.3 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415325334687634944,2461231.6985,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415325334687634944 20260710.1985 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.58 00:43:53.05 +50:11:02.3
121.69265 -12.66960 galactic Cas Second-epoch detections are separated by 4.5" and 4.7 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 414779010548775040 | 00:43:52.80 +50:11:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:53.05 +50:11:02.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:53.05 +50:11:02.3: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 53.05 +50 11 02.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414779010548775040,2461231.6985,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414779010548775040 20260710.1985 10.58CV 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 10.1985 2461231.6985 10.48 00:43:11.52 +49:49:44.5
121.56719 -13.02087 galactic Cas Second-epoch detections are separated by 0.6" 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 | Gaia DR3 414719194542686848 | 00:43:11.44 +49:49:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:11.52 +49:49:44.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:11.52 +49:49:44.5: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 11.52 +49 49 44.5 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414719194542686848,2461231.6985,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414719194542686848 20260710.1985 10.48CV 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 10.1985 2461231.6985 10.46 00:44:42.74 +49:41:44.6
121.81506 -13.16144 galactic Cas Second-epoch detections are separated by 4.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414668445209203072 | 00:44:42.40 +49:41:46.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:42.74 +49:41:44.6: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:42.74 +49:41:44.6: 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 10.1985* 00 44 42.74 +49 41 44.6 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414668445209203072,2461231.6985,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414668445209203072 20260710.1985 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.53 00:43:09.86 +50:58:24.1
121.60116 -11.87701 galactic Cas Second-epoch detections are separated by 5.2" 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 | Gaia DR3 414875840590262016 | 00:43:08.95 +50:58:28.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:09.86 +50:58:24.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:09.86 +50:58:24.1: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 09.86 +50 58 24.1 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414875840590262016,2461231.6985,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414875840590262016 20260710.1985 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 10.1985 2461231.6985 10.62 00:44:05.44 +50:43:01.4
121.74246 -12.13772 galactic Cas Second-epoch detections are separated by 3.3" and 5.0 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 414868002271153920 | 00:44:05.43 +50:43:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:05.44 +50:43:01.4: 12.24 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:05.44 +50:43:01.4: 11.96 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 05.44 +50 43 01.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414868002271153920,2461231.6985,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414868002271153920 20260710.1985 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.57 00:29:55.38 +49:08:27.7
119.31487 -13.57956 galactic Cas Second-epoch detections are separated by 6.3" and 4.6 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 J007.4798+49.1549 | 00:29:55.43 +49:08:56.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.721+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:55.38 +49:08:27.7: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:55.38 +49:08:27.7: 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 10.1985* 00 29 55.38 +49 08 27.7 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
ATO J007.4798+49.1549,2461231.6985,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J007.4798+49.1549 20260710.1985 10.57CV 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 10.1985 2461231.6985 10.51 00:38:16.02 +50:15:21.6
120.77574 -12.56060 galactic Cas Second-epoch detections are separated by 4.8" and 4.8 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 415486825457299840 | 00:38:15.90 +50:15:20.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.218+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:16.02 +50:15:21.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:16.02 +50:15:21.6: 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 10.1985* 00 38 16.02 +50 15 21.6 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415486825457299840,2461231.6985,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415486825457299840 20260710.1985 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.55 00:47:41.64 +50:48:50.0
122.32721 -12.05346 galactic Cas Second-epoch detections are separated by 6.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 415186899298963072 | 00:47:41.36 +50:48:53.7 (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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:41.64 +50:48:50.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:41.64 +50:48:50.0: 13.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 41.64 +50 48 50.0 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
Large-amplitude variable Gaia DR2 415186899298963072,2461231.6985,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415186899298963072 20260710.1985 10.55CV 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 10.1985 2461231.6985 10.62 00:41:47.49 +50:16:05.0
121.35281 -12.57411 galactic Cas Second-epoch detections are separated by 7.8" and 4.9 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 414748018065573632 | 00:41:47.56 +50:16:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:47.49 +50:16:05.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:47.49 +50:16:05.0: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 47.49 +50 16 05.0 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414748018065573632,2461231.6985,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414748018065573632 20260710.1985 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.60 00:47:16.25 +50:51:07.5
122.25951 -12.01422 galactic Cas Second-epoch detections are separated by 3.1" and 5.0 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 415187960155713664 | 00:47:16.03 +50:51:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:16.25 +50:51:07.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:16.25 +50:51:07.5: 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 10.1985* 00 47 16.25 +50 51 07.5 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415187960155713664,2461231.6985,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415187960155713664 20260710.1985 10.60CV 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 10.1985 2461231.6985 10.52 00:34:40.97 +49:51:06.3
120.16226 -12.92987 galactic Cas Second-epoch detections are separated by 3.1" and 4.7 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 J008.6772+49.8472 | 00:34:40.68 +49:51:08.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:40.97 +49:51:06.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:40.97 +49:51:06.3: 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 10.1985* 00 34 40.97 +49 51 06.3 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 J008.6772+49.8472,2461231.6985,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.6772+49.8472 20260710.1985 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.49 00:44:26.66 +49:49:48.2
121.77442 -13.02597 galactic Cas Second-epoch detections are separated by 3.8" and 5.0 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 414675763833409920 | 00:44:26.41 +49:49:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.708+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:26.66 +49:49:48.2: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:26.66 +49:49:48.2: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 26.66 +49 49 48.2 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414675763833409920,2461231.6985,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414675763833409920 20260710.1985 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.92 00:54:51.88 +56:45:46.4
123.40414 -6.10572 galactic Cas Second-epoch detections are separated by 5.2" and 4.6 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 423812155709309696 | 00:54:53.69 +56:45:14.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:54:51.88 +56:45:46.4: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:54:51.88 +56:45:46.4: 13.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 54 51.88 +56 45 46.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 423812155709309696,2461231.6985,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 423812155709309696 20260710.1985 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.55 00:49:49.28 +51:59:45.6
122.67853 -10.87495 galactic Cas Second-epoch detections are separated by 0.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J012.4643+51.9854 | 00:49:48.90 +51:59:46.7 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:49:49.28 +51:59:45.6: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:49:49.28 +51:59:45.6: 13.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 49 49.28 +51 59 45.6 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
ATO J012.4643+51.9854,2461231.6985,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012.4643+51.9854 20260710.1985 10.55CV 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 10.1985 2461231.6985 10.52 00:33:35.04 +48:58:44.3
119.91711 -13.78824 galactic Cas Second-epoch detections are separated by 4.6" 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 | Gaia DR3 391345325383616896 | 00:33:34.71 +48:58:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:35.04 +48:58:44.3: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:35.04 +48:58:44.3: 13.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 33 35.04 +48 58 44.3 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391345325383616896,2461231.6985,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391345325383616896 20260710.1985 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.51 00:36:32.00 +49:04:15.8
120.42002 -13.72799 galactic Cas Second-epoch detections are separated by 6.5" and 4.8 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 391317292136502272 | 00:36:31.67 +49:04:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:32.00 +49:04:15.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:32.00 +49:04:15.8: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 32.00 +49 04 15.8 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391317292136502272,2461231.6985,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391317292136502272 20260710.1985 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.53 00:38:25.34 +50:36:26.1
120.81974 -12.21111 galactic Cas Second-epoch detections are separated by 1.4" and 5.0 pix
The object was found in VSX 6" Gaia DR3 415520257482616448
Type: ROT
# Max. Min./Amp. JD0 Period
15.660 G 15.690 G K
ATTENTION: measured mag 10.53 is 5.1 mag brighter than the VSX record maximum brightness 15.66 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:25.34 +50:36:26.1: 12.71 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:25.34 +50:36:26.1: 12.45 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 10.1985* 00 38 25.34 +50 36 26.1 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415520257482616448,2461231.6985,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415520257482616448 20260710.1985 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 10.1985 2461231.6985 10.56 00:34:55.96 +49:03:58.2
120.15036 -13.71642 galactic Cas Second-epoch detections are separated by 5.3" and 4.9 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 J008.7403+49.0647 | 00:34:55.73 +49:03:57.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.682+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:55.96 +49:03:58.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:55.96 +49:03:58.2: 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 10.1985* 00 34 55.96 +49 03 58.2 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
ATO J008.7403+49.0647,2461231.6985,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.7403+49.0647 20260710.1985 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.59 00:39:45.58 +48:44:26.7
120.94734 -14.08599 galactic Cas Second-epoch detections are separated by 2.6" and 5.7 pix
The object was found in VSX 7" WISE J003945.5+484434
Type: EW
# Max. Min./Amp. JD0 Period
10.726 W1 Y 0.188 W1 0.554825400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:45.58 +48:44:26.7: 11.68 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:45.58 +48:44:26.7: 11.34 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.50 +/- 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 10.1985* 00 39 45.58 +48 44 26.7 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
WISE J003945.5+484434,2461231.6985,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J003945.5+484434 20260710.1985 10.59CV 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 10.1985 2461231.6985 11.43 23:08:57.49 +53:23:18.7
107.88994 -6.46372 galactic Cas Second-epoch detections are separated by 2.0" and 4.0 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 J347.2420+53.3798 | 23:08:57.49 +53:23:18.7 (user input) | SINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.340+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:08:57.49 +53:23:18.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:08:57.49 +53:23:18.7: 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 10.1985* 23 08 57.49 +53 23 18.7 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
ATO J347.2420+53.3798,2461231.6985,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.2420+53.3798 20260710.1985 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.53 00:46:17.92 +49:55:56.4
122.08342 -12.93095 galactic Cas Second-epoch detections are separated by 6.8" and 4.8 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 414757295194156800 | 00:46:17.97 +49:55:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.691+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:17.92 +49:55:56.4: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:17.92 +49:55:56.4: 13.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 17.92 +49 55 56.4 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414757295194156800,2461231.6985,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414757295194156800 20260710.1985 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 10.1985 2461231.6985 10.51 00:41:29.60 +49:57:06.5
121.29120 -12.88826 galactic Cas Second-epoch detections are separated by 4.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414736889807861504 | 00:41:29.57 +49:57:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.635+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:29.60 +49:57:06.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:29.60 +49:57:06.5: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 29.60 +49 57 06.5 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414736889807861504,2461231.6985,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414736889807861504 20260710.1985 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.55 00:43:45.45 +50:34:56.0
121.68434 -12.27092 galactic Cas Second-epoch detections are separated by 6.3" and 4.9 pix
The object was found in VSX21" Gaia DR3 414860580568711552
Type: ROT
# Max. Min./Amp. JD0 Period
16.040 G 16.070 G F
ATTENTION: measured mag 10.55 is 5.5 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:45.45 +50:34:56.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:45.45 +50:34:56.0: 13.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 45.45 +50 34 56.0 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414860580568711552,2461231.6985,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414860580568711552 20260710.1985 10.55CV 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 10.1985 2461231.6985 10.48 00:47:07.85 +50:10:53.4
122.22517 -12.68434 galactic Cas Second-epoch detections are separated by 3.9" 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 | Gaia DR3 414789249756754944 | 00:47:07.61 +50:10:54.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:07.85 +50:10:53.4: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:07.85 +50:10:53.4: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 07.85 +50 10 53.4 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414789249756754944,2461231.6985,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414789249756754944 20260710.1985 10.48CV 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 10.1985 2461231.6985 10.51 00:44:59.23 +50:13:07.3
121.87447 -12.63981 galactic Cas Second-epoch detections are separated by 4.7" and 4.9 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 J011.2432+50.2272 | 00:44:59.16 +50:13:07.7 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.388+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:59.23 +50:13:07.3: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:59.23 +50:13:07.3: 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 10.1985* 00 44 59.23 +50 13 07.3 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 J011.2432+50.2272,2461231.6985,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.2432+50.2272 20260710.1985 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.12 23:35:49.76 +51:16:44.8
111.06331 -9.84192 galactic Cas Second-epoch detections are separated by 1.6" and 4.6 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 J353.9677+51.2879 | 23:35:49.76 +51:16:44.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:35:49.76 +51:16:44.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:35:49.76 +51:16:44.8: 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 10.1985* 23 35 49.76 +51 16 44.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.9677+51.2879,2461231.6985,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J353.9677+51.2879 20260710.1985 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.88 00:48:23.17 +54:48:53.2
122.48792 -8.05434 galactic Cas Second-epoch detections are separated by 4.2" and 5.0 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 417549062599076736 | 00:48:25.85 +54:48:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:23.17 +54:48:53.2: 12.54 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:23.17 +54:48:53.2: 12.26 +/- 0.15 detection
Forced photometry reference-image weighted average: 12.41 +/- 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 10.1985* 00 48 23.17 +54 48 53.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 417549062599076736,2461231.6985,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 417549062599076736 20260710.1985 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.42 00:46:00.47 +49:48:02.8
122.03248 -13.06149 galactic Cas Second-epoch detections are separated by 6.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414754821295585536 | 00:46:00.19 +49:48:05.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:00.47 +49:48:02.8: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:00.47 +49:48:02.8: 13.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 00.47 +49 48 02.8 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414754821295585536,2461231.6985,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414754821295585536 20260710.1985 10.42CV 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 10.1985 2461231.6985 10.47 00:38:33.21 +48:51:35.5
120.74889 -13.95727 galactic Cas Second-epoch detections are separated by 5.8" and 4.9 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 391296126537759104 | 00:38:32.69 +48:51:37.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:33.21 +48:51:35.5: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:33.21 +48:51:35.5: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 33.21 +48 51 35.5 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391296126537759104,2461231.6985,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391296126537759104 20260710.1985 10.47CV 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 10.1985 2461231.6985 10.66 00:29:32.59 +48:52:54.5
119.22789 -13.83241 galactic Cas Second-epoch detections are separated by 5.1" and 5.0 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 391144428292220160 | 00:29:32.33 +48:52:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:32.59 +48:52:54.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:32.59 +48:52:54.5: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 29 32.59 +48 52 54.5 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391144428292220160,2461231.6985,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391144428292220160 20260710.1985 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.51 00:43:06.12 +50:04:43.7
121.56081 -12.77075 galactic Cas Second-epoch detections are separated by 3.8" and 4.8 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 414730395817276544 | 00:43:05.87 +50:04:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:06.12 +50:04:43.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:06.12 +50:04:43.7: 12.71 +/- 0.22 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 06.12 +50 04 43.7 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
Gaia DR3 414730395817276544,2461231.6985,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414730395817276544 20260710.1985 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.62 00:44:09.72 +50:56:04.3
121.76043 -11.92067 galactic Cas Second-epoch detections are separated by 6.6" and 4.9 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 415247063203647488 | 00:44:08.63 +50:56:13.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:09.72 +50:56:04.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:09.72 +50:56:04.3: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 09.72 +50 56 04.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415247063203647488,2461231.6985,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415247063203647488 20260710.1985 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.57 00:41:42.76 +49:30:08.8
121.30948 -13.33867 galactic Cas Second-epoch detections are separated by 4.7" and 4.6 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 414688610076367232 | 00:41:42.59 +49:30:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:42.76 +49:30:08.8: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:42.76 +49:30:08.8: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 42.76 +49 30 08.8 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414688610076367232,2461231.6985,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414688610076367232 20260710.1985 10.57CV 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 10.1985 2461231.6985 10.73 00:32:51.73 +50:26:51.0
119.90699 -12.31511 galactic Cas Second-epoch detections are separated by 3.7" and 4.6 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 391721019062047360 | 00:32:54.13 +50:26:14.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:32:51.73 +50:26:51.0: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:32:51.73 +50:26:51.0: 13.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 32 51.73 +50 26 51.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391721019062047360,2461231.6985,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391721019062047360 20260710.1985 10.73CV 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 10.1985 2461231.6985 10.42 00:40:05.03 +49:06:39.4
121.01969 -13.71864 galactic Cas Second-epoch detections are separated by 4.4" 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 | Gaia DR3 390648342389694592 | 00:40:04.64 +49:06:41.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:05.03 +49:06:39.4: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:05.03 +49:06:39.4: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 40 05.03 +49 06 39.4 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390648342389694592,2461231.6985,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390648342389694592 20260710.1985 10.42CV 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 10.1985 2461231.6985 10.62 00:38:46.06 +50:08:08.9
120.85141 -12.68475 galactic Cas Second-epoch detections are separated by 3.0" 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 J009.7086+50.1339 | 00:38:46.07 +50:08:09.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.675+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:46.06 +50:08:08.9: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:46.06 +50:08:08.9: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 46.06 +50 08 08.9 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
ATO J009.7086+50.1339,2461231.6985,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.7086+50.1339 20260710.1985 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.61 00:43:31.49 +50:48:15.7
121.65370 -12.04775 galactic Cas Second-epoch detections are separated by 5.8" 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 | Gaia DR3 414872232817760896 | 00:43:31.53 +50:48:19.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:31.49 +50:48:15.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:31.49 +50:48:15.7: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 31.49 +50 48 15.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414872232817760896,2461231.6985,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414872232817760896 20260710.1985 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.53 00:43:50.67 +49:59:41.7
121.68029 -12.85838 galactic Cas Second-epoch detections are separated by 1.0" 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 414682223464136576 | 00:43:50.38 +49:59:41.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:50.67 +49:59:41.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:50.67 +49:59:41.7: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 50.67 +49 59 41.7 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
Gaia DR3 414682223464136576,2461231.6985,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414682223464136576 20260710.1985 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 10.1985 2461231.6985 10.67 00:48:19.07 +50:56:33.0
122.42959 -11.92621 galactic Cas Second-epoch detections are separated by 8.0" and 4.9 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 415025030573893248 | 00:48:18.83 +50:56:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:19.07 +50:56:33.0: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:19.07 +50:56:33.0: 13.18 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 48 19.07 +50 56 33.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415025030573893248,2461231.6985,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415025030573893248 20260710.1985 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.58 00:36:40.92 +49:23:46.2
120.46474 -13.40488 galactic Cas Second-epoch detections are separated by 1.5" and 4.9 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 391416454341298560 | 00:36:42.82 +49:24:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.654+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:40.92 +49:23:46.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:40.92 +49:23:46.2: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 40.92 +49 23 46.2 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391416454341298560,2461231.6985,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391416454341298560 20260710.1985 10.58CV 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 10.1985 2461231.6985 11.17 00:02:36.41 +55:35:39.4
116.02330 -6.62110 galactic Cas Second-epoch detections are separated by 2.5" and 4.1 pix
The object was found in VSX23" Gaia DR3 420504687295007616
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.520 G 14.560 G A
ATTENTION: measured mag 11.17 is 3.3 mag brighter than the VSX record maximum brightness 14.52 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:02:36.41 +55:35:39.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:02:36.41 +55:35:39.4: 13.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 02 36.41 +55 35 39.4 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420504687295007616,2461231.6985,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 420504687295007616 20260710.1985 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 10.1985 2461231.6985 10.67 00:43:11.46 +50:19:29.1
121.58371 -12.52541 galactic Cas Second-epoch detections are separated by 3.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J010.7982+50.3244 | 00:43:11.46 +50:19:29.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.367+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:11.46 +50:19:29.1: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:11.46 +50:19:29.1: 13.18 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 11.46 +50 19 29.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.7982+50.3244,2461231.6985,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.7982+50.3244 20260710.1985 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.54 00:46:14.54 +50:13:40.4
122.08039 -12.63527 galactic Cas Second-epoch detections are separated by 3.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414793067980841728 | 00:46:14.21 +50:13:40.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:14.54 +50:13:40.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:14.54 +50:13:40.4: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 14.54 +50 13 40.4 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414793067980841728,2461231.6985,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414793067980841728 20260710.1985 10.54CV 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 10.1985 2461231.6985 10.74 00:39:37.61 +49:41:10.3
120.97067 -13.14057 galactic Cas Second-epoch detections are separated by 2.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391437654300032384 | 00:39:37.76 +49:41:10.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.657+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:37.61 +49:41:10.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:37.61 +49:41:10.3: 13.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 37.61 +49 41 10.3 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391437654300032384,2461231.6985,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391437654300032384 20260710.1985 10.74CV 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 10.1985 2461231.6985 10.64 00:36:02.81 +49:16:40.5
120.35123 -13.51669 galactic Cas Second-epoch detections are separated by 2.5" 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 | ATO J009.0112+49.2787 | 00:36:02.70 +49:16:43.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:02.81 +49:16:40.5: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:02.81 +49:16:40.5: 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 10.1985* 00 36 02.81 +49 16 40.5 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J009.0112+49.2787,2461231.6985,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.0112+49.2787 20260710.1985 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 10.1985 2461231.6985 10.61 00:43:49.95 +50:02:21.8
121.67969 -12.81387 galactic Cas Second-epoch detections are separated by 1.0" 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 414682768920811392 | 00:43:49.69 +50:02:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.726+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:49.95 +50:02:21.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:49.95 +50:02:21.8: 13.11 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 10.1985* 00 43 49.95 +50 02 21.8 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414682768920811392,2461231.6985,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414682768920811392 20260710.1985 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.96 00:56:43.95 +57:23:36.4
123.64841 -5.47094 galactic Cas Second-epoch detections are separated by 8.0" and 4.6 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 J014.1842+57.3974 | 00:56:47.94 +57:23:58.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.811+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:56:43.95 +57:23:36.4: 12.49 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:56:43.95 +57:23:36.4: 12.20 +/- 0.18 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 10.1985* 00 56 43.95 +57 23 36.4 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J014.1842+57.3974,2461231.6985,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J014.1842+57.3974 20260710.1985 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.64 00:36:35.81 +49:27:25.3
120.45422 -13.34331 galactic Cas Second-epoch detections are separated by 3.0" and 4.7 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 391417107176302208 | 00:36:35.64 +49:27:26.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.610+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:35.81 +49:27:25.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:35.81 +49:27:25.3: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 35.81 +49 27 25.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391417107176302208,2461231.6985,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391417107176302208 20260710.1985 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 10.1985 2461231.6985 10.60 00:36:46.61 +49:32:55.0
120.48973 -13.25360 galactic Cas Second-epoch detections are separated by 3.6" 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 | ATO J009.1936+49.5487 | 00:36:46.49 +49:32:55.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.512+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:46.61 +49:32:55.0: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:46.61 +49:32:55.0: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 46.61 +49 32 55.0 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
ATO J009.1936+49.5487,2461231.6985,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.1936+49.5487 20260710.1985 10.60CV 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 10.1985 2461231.6985 10.68 00:41:12.81 +49:20:24.3
121.21945 -13.49767 galactic Cas Second-epoch detections are separated by 5.2" 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 | Gaia DR3 390678510239921408 | 00:41:12.62 +49:20:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:12.81 +49:20:24.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:12.81 +49:20:24.3: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 12.81 +49 20 24.3 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390678510239921408,2461231.6985,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390678510239921408 20260710.1985 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.74 00:37:52.79 +49:45:39.9
120.68504 -13.05151 galactic Cas Second-epoch detections are separated by 1.4" 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 | ATO J009.4688+49.7570 | 00:37:52.55 +49:45:39.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:52.79 +49:45:39.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:52.79 +49:45:39.9: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 37 52.79 +49 45 39.9 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J009.4688+49.7570,2461231.6985,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.4688+49.7570 20260710.1985 10.74CV 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 10.1985 2461231.6985 10.58 00:44:04.96 +50:24:35.5
121.73198 -12.44475 galactic Cas Second-epoch detections are separated by 4.6" and 4.6 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 414787944080739840 | 00:44:06.61 +50:24:35.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:04.96 +50:24:35.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:04.96 +50:24:35.5: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 04.96 +50 24 35.5 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414787944080739840,2461231.6985,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414787944080739840 20260710.1985 10.58CV 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 10.1985 2461231.6985 11.50 23:25:05.02 +55:05:34.3
110.71549 -5.71749 galactic Cas Second-epoch detections are separated by 2.0" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:05.02 +55:05:34.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.363+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:05.02 +55:05:34.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:05.02 +55:05:34.3: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 23 25 05.02 +55 05 34.3 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
target,2461231.6985,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 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 10.1985 2461231.6985 10.77 00:41:28.09 +50:30:28.5
121.30965 -12.33243 galactic Cas Second-epoch detections are separated by 2.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J010.3545+50.4995 | 00:41:27.85 +50:30:29.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:28.09 +50:30:28.5: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:28.09 +50:30:28.5: 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 10.1985* 00 41 28.09 +50 30 28.5 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 J010.3545+50.4995,2461231.6985,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.3545+50.4995 20260710.1985 10.77CV 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 10.1985 2461231.6985 10.67 00:42:59.23 +50:16:22.0
121.54861 -12.57627 galactic Cas Second-epoch detections are separated by 1.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J010.7419+50.2765 | 00:42:59.19 +50:16:21.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.440+/-0.026 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:59.23 +50:16:22.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:59.23 +50:16:22.0: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 59.23 +50 16 22.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.7419+50.2765,2461231.6985,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.7419+50.2765 20260710.1985 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.74 00:39:41.88 +50:10:46.9
121.00614 -12.64815 galactic Cas Second-epoch detections are separated by 3.5" and 4.7 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 415493697405019520 | 00:39:41.90 +50:10:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.234+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:41.88 +50:10:46.9: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:41.88 +50:10:46.9: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 41.88 +50 10 46.9 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415493697405019520,2461231.6985,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415493697405019520 20260710.1985 10.74CV 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 10.1985 2461231.6985 10.72 00:33:40.12 +49:45:25.6
119.98806 -13.01304 galactic Cas Second-epoch detections are separated by 2.7" and 4.8 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 J008.4221+49.7632 | 00:33:39.88 +49:45:26.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:40.12 +49:45:25.6: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:40.12 +49:45:25.6: 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 10.1985* 00 33 40.12 +49 45 25.6 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.4221+49.7632,2461231.6985,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.4221+49.7632 20260710.1985 10.72CV 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 10.1985 2461231.6985 11.08 00:50:42.09 +57:57:35.7
122.83389 -4.91169 galactic Cas Second-epoch detections are separated by 6.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 424319752126180352 | 00:50:43.93 +57:57:10.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:50:42.09 +57:57:35.7: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:50:42.09 +57:57:35.7: 13.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 50 42.09 +57 57 35.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 424319752126180352,2461231.6985,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 424319752126180352 20260710.1985 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.84 00:35:45.67 +49:13:52.9
120.30040 -13.56027 galactic Cas Second-epoch detections are separated by 3.7" 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 | ATO J008.9393+49.2307 | 00:35:45.45 +49:13:50.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:45.67 +49:13:52.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:45.67 +49:13:52.9: 13.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 45.67 +49 13 52.9 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 J008.9393+49.2307,2461231.6985,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.9393+49.2307 20260710.1985 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.80 00:41:29.77 +50:40:23.7
121.32089 -12.16740 galactic Cas Second-epoch detections are separated by 0.8" 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 | Gaia DR3 414855392246979712 | 00:41:29.51 +50:40:23.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:29.77 +50:40:23.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:29.77 +50:40:23.7: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 29.77 +50 40 23.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414855392246979712,2461231.6985,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414855392246979712 20260710.1985 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.64 23:08:22.62 +55:49:47.2
108.76229 -4.18064 galactic Cas Second-epoch detections are separated by 1.9" and 3.9 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 J347.0951+55.8319 | 23:08:27.40 +55:49:45.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1928AnHar.100...49C HD 240196
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:08:22.62 +55:49:47.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:08:22.62 +55:49:47.2: 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 10.1985* 23 08 22.62 +55 49 47.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.0951+55.8319,2461231.6985,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.0951+55.8319 20260710.1985 11.64CV 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 10.1985 2461231.6985 10.70 00:42:57.24 +50:03:47.4
121.53593 -12.78558 galactic Cas Second-epoch detections are separated by 4.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414729124506961152 | 00:42:56.99 +50:03:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.287+/-0.027 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:57.24 +50:03:47.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:57.24 +50:03:47.4: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 57.24 +50 03 47.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414729124506961152,2461231.6985,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414729124506961152 20260710.1985 10.70CV 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 10.1985 2461231.6985 10.77 00:36:14.23 +49:21:55.9
120.38856 -13.43114 galactic Cas Second-epoch detections are separated by 3.5" and 4.5 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 391461568677785856 | 00:36:14.10 +49:21:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.561+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:14.23 +49:21:55.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:14.23 +49:21:55.9: 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 10.1985* 00 36 14.23 +49 21 55.9 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 391461568677785856,2461231.6985,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391461568677785856 20260710.1985 10.77CV 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 10.1985 2461231.6985 10.70 00:48:48.54 +51:15:20.3
122.51200 -11.61397 galactic Cas Second-epoch detections are separated by 3.0" and 5.2 pix
The object was found in VSX14" Gaia DR3 415128483447633920
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.280 G 12.310 G 0.079988400000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:48.54 +51:15:20.3: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:48.54 +51:15:20.3: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 48 48.54 +51 15 20.3 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415128483447633920,2461231.6985,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415128483447633920 20260710.1985 10.70CV 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 10.1985 2461231.6985 10.66 00:31:10.03 +49:14:57.5
119.53249 -13.48860 galactic Cas Second-epoch detections are separated by 5.5" and 4.6 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 J007.7981+49.2513 | 00:31:09.78 +49:14:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.673+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:10.03 +49:14:57.5: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:10.03 +49:14:57.5: 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 10.1985* 00 31 10.03 +49 14 57.5 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J007.7981+49.2513,2461231.6985,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J007.7981+49.2513 20260710.1985 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.65 00:36:55.44 +48:50:41.1
120.47225 -13.95767 galactic Cas Second-epoch detections are separated by 6.9" 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 | Gaia DR3 391304544673642752 | 00:36:54.97 +48:50:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:55.44 +48:50:41.1: 13.17 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:55.44 +48:50:41.1: 12.99 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 10.1985* 00 36 55.44 +48 50 41.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391304544673642752,2461231.6985,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391304544673642752 20260710.1985 10.65CV 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 10.1985 2461231.6985 10.54 00:43:50.81 +49:27:00.4
121.66374 -13.40294 galactic Cas Second-epoch detections are separated by 5.7" 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 | Gaia DR3 414643568758941696 | 00:43:50.47 +49:27:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:50.81 +49:27:00.4: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:50.81 +49:27:00.4: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 50.81 +49 27 00.4 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414643568758941696,2461231.6985,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414643568758941696 20260710.1985 10.54CV 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 10.1985 2461231.6985 10.72 00:33:05.52 +49:31:10.2
119.87489 -13.24332 galactic Cas Second-epoch detections are separated by 3.5" and 5.0 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 391575673069952640 | 00:33:05.34 +49:31:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:05.52 +49:31:10.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:05.52 +49:31:10.2: 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 10.1985* 00 33 05.52 +49 31 10.2 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391575673069952640,2461231.6985,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391575673069952640 20260710.1985 10.72CV 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 10.1985 2461231.6985 10.67 00:42:38.36 +51:09:47.4
121.52352 -11.68452 galactic Cas Second-epoch detections are separated by 5.8" and 5.0 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 415264822889360512 | 00:42:37.98 +51:09:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:38.36 +51:09:47.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:38.36 +51:09:47.4: 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 10.1985* 00 42 38.36 +51 09 47.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415264822889360512,2461231.6985,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415264822889360512 20260710.1985 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.71 00:43:42.89 +49:43:38.4
121.65047 -13.12520 galactic Cas Second-epoch detections are separated by 3.6" and 5.0 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 J010.9230+49.7257 | 00:43:42.72 +49:43:36.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.778+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:42.89 +49:43:38.4: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:42.89 +49:43:38.4: 13.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 42.89 +49 43 38.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.9230+49.7257,2461231.6985,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.9230+49.7257 20260710.1985 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.62 00:33:00.47 +49:11:35.9
119.83625 -13.56763 galactic Cas Second-epoch detections are separated by 6.6" and 4.5 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 391353507300264064 | 00:33:00.19 +49:11:36.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:00.47 +49:11:35.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:00.47 +49:11:35.9: 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 10.1985* 00 33 00.47 +49 11 35.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391353507300264064,2461231.6985,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391353507300264064 20260710.1985 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.63 00:28:15.88 +48:43:18.0
118.99704 -13.97295 galactic Cas Second-epoch detections are separated by 4.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391185110222477696 | 00:28:15.65 +48:43:17.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:15.88 +48:43:18.0: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:15.88 +48:43:18.0: 13.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 28 15.88 +48 43 18.0 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391185110222477696,2461231.6985,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391185110222477696 20260710.1985 10.63CV 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 10.1985 2461231.6985 10.77 00:37:15.82 +50:03:05.3
120.59986 -12.75608 galactic Cas Second-epoch detections are separated by 2.7" and 4.8 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 391461018921664512 | 00:37:15.88 +50:03:05.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.808+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:15.82 +50:03:05.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:15.82 +50:03:05.3: 13.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 37 15.82 +50 03 05.3 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 391461018921664512,2461231.6985,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391461018921664512 20260710.1985 10.77CV 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 10.1985 2461231.6985 11.22 23:49:50.08 +53:26:58.0
113.73449 -8.31863 galactic Cas Second-epoch detections are separated by 0.8" and 4.5 pix
The object was found in VSX15" Gaia DR3 1993447467730084096
Type: ROT
# Max. Min./Amp. JD0 Period
16.990 G 17.090 G K
ATTENTION: measured mag 11.22 is 5.8 mag brighter than the VSX record maximum brightness 16.99 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:49:50.08 +53:26:58.0: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:49:50.08 +53:26:58.0: 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 10.1985* 23 49 50.08 +53 26 58.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993447467730084096,2461231.6985,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1993447467730084096 20260710.1985 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.62 00:42:28.55 +49:30:37.3
121.43702 -13.33537 galactic Cas Second-epoch detections are separated by 3.9" 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 | Gaia DR3 414686621510854912 | 00:42:28.32 +49:30:37.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.042+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:28.55 +49:30:37.3: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:28.55 +49:30:37.3: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 28.55 +49 30 37.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414686621510854912,2461231.6985,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414686621510854912 20260710.1985 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.87 00:47:33.94 +51:22:13.1
122.31521 -11.49681 galactic Cas Second-epoch detections are separated by 5.7" and 5.1 pix
The object was found in VSX 8" Gaia DR3 415226962756827776
Type: VAR
# Max. Min./Amp. JD0 Period
12.290 G 12.310 G 0.019165500000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:33.94 +51:22:13.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:33.94 +51:22:13.1: 13.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 33.94 +51 22 13.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415226962756827776,2461231.6985,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415226962756827776 20260710.1985 10.87CV 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 10.1985 2461231.6985 10.75 00:16:11.31 +49:15:05.4
117.03611 -13.21631 galactic Cas Second-epoch detections are separated by 1.3" and 5.0 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 392915157409107968 | 00:16:13.34 +49:14:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:16:11.31 +49:15:05.4: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:16:11.31 +49:15:05.4: 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 10.1985* 00 16 11.31 +49 15 05.4 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 392915157409107968,2461231.6985,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 392915157409107968 20260710.1985 10.75CV 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 10.1985 2461231.6985 10.90 00:40:29.52 +50:01:01.3
121.12903 -12.81640 galactic Cas Second-epoch detections are separated by 4.4" and 4.9 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 414717545274956800 | 00:40:29.53 +50:01:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.044+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:29.52 +50:01:01.3: 13.56 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:29.52 +50:01:01.3: 13.27 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.56 +/- 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 10.1985* 00 40 29.52 +50 01 01.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414717545274956800,2461231.6985,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414717545274956800 20260710.1985 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.81 00:41:38.91 +50:27:39.9
121.33711 -12.38035 galactic Cas Second-epoch detections are separated by 4.7" and 4.8 pix
The object was found in VSX 1" T-Cas0-03975
Type: EA
# Max. Min./Amp. JD0 Period
12.000 R Y 0.124 R 2453275.09300 3.663730000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:38.91 +50:27:39.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:38.91 +50:27:39.9: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 38.91 +50 27 39.9 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
T-Cas0-03975,2461231.6985,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
T-Cas0-03975 20260710.1985 10.81CV 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 10.1985 2461231.6985 10.78 00:31:56.92 +49:18:09.7
119.66750 -13.44548 galactic Cas Second-epoch detections are separated by 7.4" and 5.0 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 391545715676455680 | 00:31:56.75 +49:18:08.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.581+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:56.92 +49:18:09.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:56.92 +49:18:09.7: 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 10.1985* 00 31 56.92 +49 18 09.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391545715676455680,2461231.6985,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391545715676455680 20260710.1985 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 10.1985 2461231.6985 10.80 00:44:22.71 +49:48:54.5
121.76309 -13.04059 galactic Cas Second-epoch detections are separated by 7.1" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414675793893937536 | 00:44:22.46 +49:48:56.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:22.71 +49:48:54.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:22.71 +49:48:54.5: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 22.71 +49 48 54.5 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 414675793893937536,2461231.6985,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414675793893937536 20260710.1985 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.71 00:37:42.99 +49:34:53.4
120.64792 -13.22939 galactic Cas Second-epoch detections are separated by 1.5" and 5.4 pix
The object was found in VSX 3" T-Cas0-03732
Type: E
# Max. Min./Amp. JD0 Period
11.685 R Y 0.207 R 2453278.79400 1.986264000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:42.99 +49:34:53.4: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:42.99 +49:34:53.4: 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 10.1985* 00 37 42.99 +49 34 53.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
T-Cas0-03732,2461231.6985,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
T-Cas0-03732 20260710.1985 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.73 00:44:34.34 +50:15:23.5
121.80755 -12.60023 galactic Cas Second-epoch detections are separated by 2.5" 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 | Gaia DR3 414784409323359872 | 00:44:34.13 +50:15:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.259+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:34.34 +50:15:23.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:34.34 +50:15:23.5: 13.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 34.34 +50 15 23.5 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414784409323359872,2461231.6985,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414784409323359872 20260710.1985 10.73CV 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 10.1985 2461231.6985 10.93 00:33:38.04 +48:56:21.0
119.92262 -13.82853 galactic Cas Second-epoch detections are separated by 6.3" 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 | Gaia DR3 391341958129257216 | 00:33:37.78 +48:56:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:38.04 +48:56:21.0: 13.43 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:38.04 +48:56:21.0: 13.27 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.43 +/- 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 10.1985* 00 33 38.04 +48 56 21.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391341958129257216,2461231.6985,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391341958129257216 20260710.1985 10.93CV 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 10.1985 2461231.6985 10.87 00:46:54.69 +50:39:25.0
122.19795 -12.20835 galactic Cas Second-epoch detections are separated by 7.0" 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 | Gaia DR3 415177725253144832 | 00:46:54.55 +50:39:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:54.69 +50:39:25.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:54.69 +50:39:25.0: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 54.69 +50 39 25.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415177725253144832,2461231.6985,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415177725253144832 20260710.1985 10.87CV 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 10.1985 2461231.6985 10.73 00:43:14.24 +49:38:10.6
121.56822 -13.21376 galactic Cas Second-epoch detections are separated by 4.1" 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 | Gaia DR3 414694141994237056 | 00:43:13.94 +49:38:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:14.24 +49:38:10.6: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:14.24 +49:38:10.6: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 14.24 +49 38 10.6 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414694141994237056,2461231.6985,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414694141994237056 20260710.1985 10.73CV 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 10.1985 2461231.6985 10.83 00:34:06.99 +49:36:32.0
120.05162 -13.16596 galactic Cas Second-epoch detections are separated by 3.4" 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 | Gaia DR3 391480363454225664 | 00:34:06.72 +49:36:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:06.99 +49:36:32.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:06.99 +49:36:32.0: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 06.99 +49 36 32.0 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391480363454225664,2461231.6985,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391480363454225664 20260710.1985 10.83CV 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 10.1985 2461231.6985 10.79 00:41:52.51 +49:45:52.2
121.34684 -13.07782 galactic Cas Second-epoch detections are separated by 5.3" and 4.6 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 414698265162833408 | 00:41:52.37 +49:45:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.760+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:52.51 +49:45:52.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:52.51 +49:45:52.2: 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 10.1985* 00 41 52.51 +49 45 52.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414698265162833408,2461231.6985,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414698265162833408 20260710.1985 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.90 00:35:41.72 +49:31:18.6
120.30812 -13.26970 galactic Cas Second-epoch detections are separated by 2.3" and 4.9 pix
The object was found in VSX 2" Gaia DR3 391465000353186688
Type: ROT
# Max. Min./Amp. JD0 Period
12.180 G 12.210 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:41.72 +49:31:18.6: 13.56 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:41.72 +49:31:18.6: 12.75 +/- 0.23 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 10.1985* 00 35 41.72 +49 31 18.6 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391465000353186688,2461231.6985,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391465000353186688 20260710.1985 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.62 00:38:37.19 +48:53:14.6
120.76158 -13.93034 galactic Cas Second-epoch detections are separated by 5.2" 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 | ATO J009.6514+48.8855 | 00:38:36.80 +48:53:19.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:37.19 +48:53:14.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:37.19 +48:53:14.6: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 37.19 +48 53 14.6 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
ATO J009.6514+48.8855,2461231.6985,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.6514+48.8855 20260710.1985 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.88 00:42:06.28 +50:45:22.0
121.42258 -12.08828 galactic Cas Second-epoch detections are separated by 3.1" and 5.0 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 414877691717178752 | 00:42:06.16 +50:45:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.291+/-0.039 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:06.28 +50:45:22.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:06.28 +50:45:22.0: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 06.28 +50 45 22.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414877691717178752,2461231.6985,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414877691717178752 20260710.1985 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.85 00:49:00.11 +51:55:18.7
122.54935 -10.94808 galactic Cas Second-epoch detections are separated by 3.2" 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 | Gaia DR3 415361137535102080 | 00:48:59.99 +51:55:21.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:49:00.11 +51:55:18.7: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:49:00.11 +51:55:18.7: 13.15 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 10.1985* 00 49 00.11 +51 55 18.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415361137535102080,2461231.6985,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415361137535102080 20260710.1985 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.78 00:35:10.25 +49:13:30.4
120.20105 -13.56036 galactic Cas Second-epoch detections are separated by 3.9" and 5.4 pix
The object was found in VSX 2" Gaia DR3 391363334181923072
Type: ROT
# Max. Min./Amp. JD0 Period
12.110 G 12.140 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:10.25 +49:13:30.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:10.25 +49:13:30.4: 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 10.1985* 00 35 10.25 +49 13 30.4 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 391363334181923072,2461231.6985,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391363334181923072 20260710.1985 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 10.1985 2461231.6985 10.89 00:45:35.04 +50:06:54.9
121.96982 -12.74556 galactic Cas Second-epoch detections are separated by 3.4" 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 | Gaia DR3 414768118511738112 | 00:45:34.91 +50:06:55.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.881+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:35.04 +50:06:54.9: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:35.04 +50:06:54.9: 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 10.1985* 00 45 35.04 +50 06 54.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414768118511738112,2461231.6985,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414768118511738112 20260710.1985 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.89 00:41:50.04 +50:11:56.9
121.35707 -12.64324 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 | Gaia DR3 414745509804674432 | 00:41:49.90 +50:11:54.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:50.04 +50:11:56.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:50.04 +50:11:56.9: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 50.04 +50 11 56.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414745509804674432,2461231.6985,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414745509804674432 20260710.1985 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.79 00:43:26.77 +50:14:20.5
121.62262 -12.61240 galactic Cas Second-epoch detections are separated by 5.1" and 4.8 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 414825572293286400 | 00:43:26.62 +50:14:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.213+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:26.77 +50:14:20.5: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:26.77 +50:14:20.5: 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 10.1985* 00 43 26.77 +50 14 20.5 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 414825572293286400,2461231.6985,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414825572293286400 20260710.1985 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.57 23:16:02.64 +53:58:02.4
109.08705 -6.32029 galactic Cas Second-epoch detections are separated by 0.9" and 4.3 pix
The object was found in VSX 3" Gaia DR3 1995961982102744192
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.260 G 13.300 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:16:02.64 +53:58:02.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:16:02.64 +53:58:02.4: 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 10.1985* 23 16 02.64 +53 58 02.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995961982102744192,2461231.6985,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1995961982102744192 20260710.1985 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 10.1985 2461231.6985 10.85 00:44:12.55 +50:33:09.4
121.75681 -12.30264 galactic Cas Second-epoch detections are separated by 4.2" and 5.2 pix
The object was found in VSX 3" Gaia DR3 414859515415752960
Type: ROT
# Max. Min./Amp. JD0 Period
12.340 G 12.370 G 3.684440000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:12.55 +50:33:09.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:12.55 +50:33:09.4: 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 10.1985* 00 44 12.55 +50 33 09.4 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 414859515415752960,2461231.6985,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414859515415752960 20260710.1985 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.78 00:40:26.52 +49:52:04.2
121.11409 -12.96510 galactic Cas Second-epoch detections are separated by 4.2" and 5.0 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 414714963995673088 | 00:40:26.36 +49:52:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:26.52 +49:52:04.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:26.52 +49:52:04.2: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 40 26.52 +49 52 04.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414714963995673088,2461231.6985,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414714963995673088 20260710.1985 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 10.1985 2461231.6985 10.81 00:40:17.36 +49:38:27.2
121.07852 -13.19074 galactic Cas Second-epoch detections are separated by 2.8" 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 | Gaia DR3 390686855357530368 | 00:40:17.24 +49:38:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.757+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:17.36 +49:38:27.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:17.36 +49:38:27.2: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 40 17.36 +49 38 27.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390686855357530368,2461231.6985,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390686855357530368 20260710.1985 10.81CV 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 10.1985 2461231.6985 10.72 00:46:08.11 +50:17:34.9
122.06423 -12.56979 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 | Gaia DR3 414793888320720128 | 00:46:07.79 +50:17:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:08.11 +50:17:34.9: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:08.11 +50:17:34.9: 13.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 08.11 +50 17 34.9 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414793888320720128,2461231.6985,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414793888320720128 20260710.1985 10.72CV 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 10.1985 2461231.6985 10.83 00:36:53.34 +49:27:42.2
120.50321 -13.34141 galactic Cas Second-epoch detections are separated by 1.0" and 5.0 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 J009.2175+49.4637 | 00:36:53.12 +49:27:43.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:53.34 +49:27:42.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:53.34 +49:27:42.2: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 53.34 +49 27 42.2 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 J009.2175+49.4637,2461231.6985,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.2175+49.4637 20260710.1985 10.83CV 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 10.1985 2461231.6985 10.79 00:47:01.70 +50:42:52.3
122.21793 -12.15111 galactic Cas Second-epoch detections are separated by 4.2" and 5.0 pix
The object was found in VSX 5" Gaia DR3 415179408879228800
Type: VAR
# Max. Min./Amp. JD0 Period
12.190 G 12.210 G 0.031261500000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:01.70 +50:42:52.3: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:01.70 +50:42:52.3: 12.88 +/- 0.27 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 10.1985* 00 47 01.70 +50 42 52.3 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 415179408879228800,2461231.6985,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415179408879228800 20260710.1985 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.74 00:38:01.64 +49:00:50.7
120.66836 -13.79872 galactic Cas Second-epoch detections are separated by 3.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391302105132172928 | 00:38:01.32 +49:00:51.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:01.64 +49:00:50.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:01.64 +49:00:50.7: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 01.64 +49 00 50.7 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391302105132172928,2461231.6985,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391302105132172928 20260710.1985 10.74CV 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 10.1985 2461231.6985 10.79 00:49:38.43 +51:51:57.0
122.64924 -11.00493 galactic Cas Second-epoch detections are separated by 0.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 415172983607963904 | 00:49:38.19 +51:51:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:49:38.43 +51:51:57.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:49:38.43 +51:51:57.0: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 49 38.43 +51 51 57.0 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415172983607963904,2461231.6985,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415172983607963904 20260710.1985 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.89 00:47:48.94 +51:15:14.7
122.35332 -11.61360 galactic Cas Second-epoch detections are separated by 7.6" 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 | Gaia DR3 415223183185665024 | 00:47:48.36 +51:15:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:48.94 +51:15:14.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:48.94 +51:15:14.7: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 48.94 +51 15 14.7 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415223183185665024,2461231.6985,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415223183185665024 20260710.1985 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.77 00:41:59.49 +49:46:29.2
121.36651 -13.06826 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 | Gaia DR3 414699575132087040 | 00:41:59.44 +49:46:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:59.49 +49:46:29.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:59.49 +49:46:29.2: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 59.49 +49 46 29.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414699575132087040,2461231.6985,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414699575132087040 20260710.1985 10.77CV 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 10.1985 2461231.6985 10.69 00:43:19.16 +49:55:12.4
121.59128 -12.93050 galactic Cas Second-epoch detections are separated by 5.0" and 4.6 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 414721393565900544 | 00:43:19.03 +49:55:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.689+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:19.16 +49:55:12.4: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:19.16 +49:55:12.4: 13.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 19.16 +49 55 12.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414721393565900544,2461231.6985,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414721393565900544 20260710.1985 10.69CV 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 10.1985 2461231.6985 10.84 00:34:00.17 +49:37:27.3
120.03385 -13.14937 galactic Cas Second-epoch detections are separated by 2.9" and 5.0 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 J008.4995+49.6254 | 00:33:59.88 +49:37:31.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:00.17 +49:37:27.3: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:00.17 +49:37:27.3: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 00.17 +49 37 27.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.4995+49.6254,2461231.6985,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.4995+49.6254 20260710.1985 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.73 00:46:15.15 +49:37:46.0
122.06937 -13.23362 galactic Cas Second-epoch detections are separated by 7.3" and 5.0 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 414657656251648384 | 00:46:14.97 +49:37:47.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.020+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:15.15 +49:37:46.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:15.15 +49:37:46.0: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 15.15 +49 37 46.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414657656251648384,2461231.6985,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414657656251648384 20260710.1985 10.73CV 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 10.1985 2461231.6985 10.85 00:44:08.70 +49:37:08.8
121.71859 -13.23546 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 | Gaia DR3 414666899021006464 | 00:44:08.33 +49:37:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:08.70 +49:37:08.8: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:08.70 +49:37:08.8: 13.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 08.70 +49 37 08.8 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 414666899021006464,2461231.6985,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414666899021006464 20260710.1985 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.83 00:41:18.79 +50:23:11.4
121.27944 -12.45276 galactic Cas Second-epoch detections are separated by 3.4" and 4.9 pix
The object was found in VSX 4" Gaia DR3 414751935075744256
Type: VAR
# Max. Min./Amp. JD0 Period
12.280 G 12.290 G 0.063309000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:18.79 +50:23:11.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:18.79 +50:23:11.4: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 18.79 +50 23 11.4 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 414751935075744256,2461231.6985,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414751935075744256 20260710.1985 10.83CV 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 10.1985 2461231.6985 10.87 00:46:30.01 +51:10:00.8
122.14148 -11.69728 galactic Cas Second-epoch detections are separated by 8.6" 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 415229161780168704 | 00:46:29.42 +51:10:07.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:30.01 +51:10:00.8: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:30.01 +51:10:00.8: 13.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 30.01 +51 10 00.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415229161780168704,2461231.6985,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415229161780168704 20260710.1985 10.87CV 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 10.1985 2461231.6985 10.85 00:46:45.82 +50:14:20.7
122.16603 -12.62571 galactic Cas Second-epoch detections are separated by 3.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414790387921498240 | 00:46:45.56 +50:14:19.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:45.82 +50:14:20.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:45.82 +50:14:20.7: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 45.82 +50 14 20.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414790387921498240,2461231.6985,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414790387921498240 20260710.1985 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.81 00:39:13.54 +49:40:17.3
120.90338 -13.15217 galactic Cas Second-epoch detections are separated by 1.0" 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 | Gaia DR3 391437065885060480 | 00:39:13.39 +49:40:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:13.54 +49:40:17.3: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:13.54 +49:40:17.3: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 13.54 +49 40 17.3 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 391437065885060480,2461231.6985,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391437065885060480 20260710.1985 10.81CV 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 10.1985 2461231.6985 10.90 00:28:11.92 +49:22:01.3
119.04744 -13.32936 galactic Cas Second-epoch detections are separated by 6.9" and 4.5 pix
The object was found in VSX 3" Gaia DR3 391230254621584000
Type: VAR
# Max. Min./Amp. JD0 Period
12.410 G 12.430 G 0.031272100000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:11.92 +49:22:01.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:11.92 +49:22:01.3: 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 10.1985* 00 28 11.92 +49 22 01.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391230254621584000,2461231.6985,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391230254621584000 20260710.1985 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.81 00:38:16.15 +49:02:55.2
120.71101 -13.76629 galactic Cas Second-epoch detections are separated by 8.3" and 4.4 pix
The object was found in VSX 4" Gaia DR3 391301791595715584
Type: VAR
# Max. Min./Amp. JD0 Period
12.150 G 12.160 G 0.025736500000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:16.15 +49:02:55.2: 13.37 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:16.15 +49:02:55.2: 13.04 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 10.1985* 00 38 16.15 +49 02 55.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391301791595715584,2461231.6985,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391301791595715584 20260710.1985 10.81CV 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 10.1985 2461231.6985 11.53 23:29:14.19 +53:24:27.1
110.74710 -7.50833 galactic Cas Second-epoch detections are separated by 3.2" and 4.3 pix
The object was found in VSX25" Gaia DR3 1992558581298399104
Type: ROT
# Max. Min./Amp. JD0 Period
15.670 G 15.710 G K
ATTENTION: measured mag 11.53 is 4.1 mag brighter than the VSX record maximum brightness 15.67 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:29:14.19 +53:24:27.1: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:29:14.19 +53:24:27.1: 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 10.1985* 23 29 14.19 +53 24 27.1 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
Gaia DR3 1992558581298399104,2461231.6985,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1992558581298399104 20260710.1985 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.89 00:47:56.81 +51:05:58.0
122.37209 -11.76851 galactic Cas Second-epoch detections are separated by 7.6" and 5.0 pix
The object was found in VSX 5" Gaia DR3 415219919010814720
Type: VAR
# Max. Min./Amp. JD0 Period
12.140 G 12.150 G 0.042395800000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:56.81 +51:05:58.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:56.81 +51:05:58.0: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 56.81 +51 05 58.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415219919010814720,2461231.6985,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415219919010814720 20260710.1985 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.92 00:42:02.11 +50:39:27.8
121.40759 -12.18619 galactic Cas Second-epoch detections are separated by 5.4" and 4.6 pix
The object was found in VSX16" Gaia DR3 414853541119876736
Type: RS
# Max. Min./Amp. JD0 Period
14.270 G 14.340 G K
ATTENTION: measured mag 10.92 is 3.3 mag brighter than the VSX record maximum brightness 14.27 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:02.11 +50:39:27.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:02.11 +50:39:27.8: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 02.11 +50 39 27.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414853541119876736,2461231.6985,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414853541119876736 20260710.1985 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.38 00:47:00.30 +58:07:18.8
122.34466 -4.74481 galactic Cas Second-epoch detections are separated by 6.5" and 4.5 pix
The object was found in VSX 3" Gaia DR3 425084943497523584
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.900 G 12.930 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:00.30 +58:07:18.8: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:00.30 +58:07:18.8: 12.94 +/- 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 10.1985* 00 47 00.30 +58 07 18.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 425084943497523584,2461231.6985,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 425084943497523584 20260710.1985 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.04 00:37:00.43 +48:58:17.9
120.49386 -13.83178 galactic Cas Second-epoch detections are separated by 0.6" 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 391307156013714688 | 00:37:00.22 +48:58:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:00.43 +48:58:17.9: 13.26 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:00.43 +48:58:17.9: 12.88 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 37 00.43 +48 58 17.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391307156013714688,2461231.6985,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391307156013714688 20260710.1985 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.89 00:35:14.12 +50:03:26.3
120.26703 -12.73059 galactic Cas Second-epoch detections are separated by 2.9" and 4.8 pix
The object was found in VSX23" Gaia DR3 391516853496480384
Type: RS
# Max. Min./Amp. JD0 Period
14.030 G 14.090 G 0.364822000000 A
ATTENTION: measured mag 10.89 is 3.1 mag brighter than the VSX record maximum brightness 14.03 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:14.12 +50:03:26.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:14.12 +50:03:26.3: 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 10.1985* 00 35 14.12 +50 03 26.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391516853496480384,2461231.6985,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391516853496480384 20260710.1985 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.76 00:45:54.99 +50:24:54.3
122.03120 -12.44701 galactic Cas Second-epoch detections are separated by 2.5" 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 | ATO J011.4621+50.4197 | 00:45:54.79 +50:24:53.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.743+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:54.99 +50:24:54.3: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:54.99 +50:24:54.3: 13.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 54.99 +50 24 54.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J011.4621+50.4197,2461231.6985,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.4621+50.4197 20260710.1985 10.76CV 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 10.1985 2461231.6985 11.04 00:41:00.79 +49:46:02.8
121.20417 -13.06933 galactic Cas Second-epoch detections are separated by 1.7" 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 | Gaia DR3 414704862232599936 | 00:41:00.68 +49:46:03.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:00.79 +49:46:02.8: 12.98 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:00.79 +49:46:02.8: 13.23 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.98 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 00.79 +49 46 02.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414704862232599936,2461231.6985,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414704862232599936 20260710.1985 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.85 00:37:13.07 +50:18:04.1
120.60680 -12.50640 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 | Gaia DR3 415489333717934848 | 00:37:13.09 +50:18:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.201+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:13.07 +50:18:04.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:13.07 +50:18:04.1: 13.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 37 13.07 +50 18 04.1 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 415489333717934848,2461231.6985,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415489333717934848 20260710.1985 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.95 00:40:07.31 +50:28:21.6
121.08912 -12.35859 galactic Cas Second-epoch detections are separated by 1.6" 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 | Gaia DR3 415504452005180672 | 00:40:07.28 +50:28:19.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.259+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:07.31 +50:28:21.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:07.31 +50:28:21.6: 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 10.1985* 00 40 07.31 +50 28 21.6 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415504452005180672,2461231.6985,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415504452005180672 20260710.1985 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.06 00:44:56.27 +50:15:32.7
121.86746 -12.59923 galactic Cas Second-epoch detections are separated by 5.5" and 4.7 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 414781862407057152 | 00:44:56.01 +50:15:33.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:56.27 +50:15:32.7: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:56.27 +50:15:32.7: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 56.27 +50 15 32.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414781862407057152,2461231.6985,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414781862407057152 20260710.1985 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.89 00:39:18.87 +49:31:19.9
120.91071 -13.30197 galactic Cas Second-epoch detections are separated by 2.1" and 5.0 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 | Large-amplitude variable Gaia DR2 391430060798072576 | 00:39:18.59 +49:31:23.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:18.87 +49:31:19.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:18.87 +49:31:19.9: 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 10.1985* 00 39 18.87 +49 31 19.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 391430060798072576,2461231.6985,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391430060798072576 20260710.1985 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.06 00:29:08.31 +49:02:49.1
119.17478 -13.66203 galactic Cas Second-epoch detections are separated by 6.5" and 4.7 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 391216068346655104 | 00:29:08.12 +49:02:48.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.453+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:08.31 +49:02:49.1: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:08.31 +49:02:49.1: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 29 08.31 +49 02 49.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391216068346655104,2461231.6985,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391216068346655104 20260710.1985 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.89 00:37:51.50 +49:25:31.9
120.66282 -13.38638 galactic Cas Second-epoch detections are separated by 0.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391418344127101696 | 00:37:51.13 +49:25:33.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:51.50 +49:25:31.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:51.50 +49:25:31.9: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 37 51.50 +49 25 31.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391418344127101696,2461231.6985,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391418344127101696 20260710.1985 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.95 00:34:37.06 +49:02:32.4
120.09572 -13.73677 galactic Cas Second-epoch detections are separated by 6.5" and 4.8 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 391337530022171904 | 00:34:36.96 +49:02:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.380+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:37.06 +49:02:32.4: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:37.06 +49:02:32.4: 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 10.1985* 00 34 37.06 +49 02 32.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391337530022171904,2461231.6985,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391337530022171904 20260710.1985 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.97 00:31:47.72 +49:24:29.2
119.65037 -13.33844 galactic Cas Second-epoch detections are separated by 3.8" and 5.0 pix
The object was found in VSX 3" Gaia DR3 391548361376259200
Type: VAR
# Max. Min./Amp. JD0 Period
12.200 G 12.230 G 0.050266800000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:47.72 +49:24:29.2: 13.54 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:47.72 +49:24:29.2: 13.26 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 31 47.72 +49 24 29.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391548361376259200,2461231.6985,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391548361376259200 20260710.1985 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.03 00:46:18.71 +50:55:13.5
122.10621 -11.94311 galactic Cas Second-epoch detections are separated by 3.1" and 5.4 pix
The object was found in VSX21" Gaia DR3 415190781952545664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.690 G 13.750 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:18.71 +50:55:13.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:18.71 +50:55:13.5: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 18.71 +50 55 13.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415190781952545664,2461231.6985,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415190781952545664 20260710.1985 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.88 00:41:45.39 +49:38:15.5
121.32215 -13.20385 galactic Cas Second-epoch detections are separated by 4.2" and 4.7 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 J010.4344+49.6377 | 00:41:45.19 +49:38:16.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.328+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:45.39 +49:38:15.5: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:45.39 +49:38:15.5: 13.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 45.39 +49 38 15.5 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.4344+49.6377,2461231.6985,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.4344+49.6377 20260710.1985 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.93 00:35:42.35 +49:48:55.2
120.32876 -12.97688 galactic Cas Second-epoch detections are separated by 1.7" and 5.6 pix
The object was found in VSX 3" Gaia DR3 391477717754585984
Type: ROT
# Max. Min./Amp. JD0 Period
12.060 G 12.090 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:42.35 +49:48:55.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:42.35 +49:48:55.2: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 42.35 +49 48 55.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391477717754585984,2461231.6985,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391477717754585984 20260710.1985 10.93CV 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 10.1985 2461231.6985 10.98 00:42:08.09 +49:34:51.3
121.38286 -13.26285 galactic Cas Second-epoch detections are separated by 3.2" and 5.1 pix
The object was found in VSX 1" ASASSN-V J004207.97+493451.0
Type: SR
# Max. Min./Amp. JD0 Period
13.050 V 13.170 V 2457363.85000 39.060000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:08.09 +49:34:51.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:08.09 +49:34:51.3: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 08.09 +49 34 51.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J004207.97+493451.0,2461231.6985,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J004207.97+493451.0 20260710.1985 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 10.1985 2461231.6985 11.04 00:30:23.86 +49:14:52.6
119.40368 -13.47961 galactic Cas Second-epoch detections are separated by 3.6" and 5.0 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 391553785916297088 | 00:30:23.65 +49:14:51.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:23.86 +49:14:52.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:23.86 +49:14:52.6: 13.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 30 23.86 +49 14 52.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391553785916297088,2461231.6985,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391553785916297088 20260710.1985 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.97 00:47:38.64 +51:01:39.2
122.32242 -11.83970 galactic Cas Second-epoch detections are separated by 6.2" 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 | Gaia DR3 415214142276343808 | 00:47:37.89 +51:01:45.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:38.64 +51:01:39.2: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:38.64 +51:01:39.2: 13.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 38.64 +51 01 39.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415214142276343808,2461231.6985,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415214142276343808 20260710.1985 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.09 00:42:11.39 +49:32:38.0
121.39061 -13.30018 galactic Cas Second-epoch detections are separated by 4.9" and 4.7 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 J010.5554+49.5429 | 00:42:11.21 +49:32:40.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:11.39 +49:32:38.0: 12.93 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:11.39 +49:32:38.0: 13.23 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.93 +/- 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 10.1985* 00 42 11.39 +49 32 38.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.5554+49.5429,2461231.6985,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.5554+49.5429 20260710.1985 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.79 00:47:34.39 +50:57:36.5
122.30999 -11.90694 galactic Cas Second-epoch detections are separated by 4.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 415212084990330240 | 00:47:33.79 +50:57:42.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:34.39 +50:57:36.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:34.39 +50:57:36.5: 13.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 34.39 +50 57 36.5 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 415212084990330240,2461231.6985,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415212084990330240 20260710.1985 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.91 00:43:34.41 +49:42:59.4
121.62668 -13.13532 galactic Cas Second-epoch detections are separated by 3.0" and 5.1 pix
The object was found in VSX 3" Gaia DR3 414671155329264384
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.220 G 12.260 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:34.41 +49:42:59.4: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:34.41 +49:42:59.4: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 34.41 +49 42 59.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414671155329264384,2461231.6985,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414671155329264384 20260710.1985 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.63 23:42:21.26 +57:04:54.2
113.61766 -4.53545 galactic Cas Second-epoch detections are separated by 3.1" and 4.0 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 1997889391630039040 | 23:42:23.09 +57:04:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1928AnHar.100...49C HD 240367
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:42:21.26 +57:04:54.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:42:21.26 +57:04:54.2: 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 10.1985* 23 42 21.26 +57 04 54.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997889391630039040,2461231.6985,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1997889391630039040 20260710.1985 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.88 00:41:20.21 +49:42:43.6
121.25550 -13.12676 galactic Cas Second-epoch detections are separated by 0.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414703732660446848 | 00:41:19.99 +49:42:46.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:20.21 +49:42:43.6: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:20.21 +49:42:43.6: 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 10.1985* 00 41 20.21 +49 42 43.6 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414703732660446848,2461231.6985,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414703732660446848 20260710.1985 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.95 00:46:38.80 +50:30:06.2
122.15199 -12.36277 galactic Cas Second-epoch detections are separated by 4.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414803994377843072 | 00:46:38.56 +50:30:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:38.80 +50:30:06.2: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:38.80 +50:30:06.2: 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 10.1985* 00 46 38.80 +50 30 06.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414803994377843072,2461231.6985,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414803994377843072 20260710.1985 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.93 00:41:29.89 +50:21:53.2
121.30874 -12.47564 galactic Cas Second-epoch detections are separated by 1.9" and 5.0 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 | Large-amplitude variable Gaia DR2 414748915712338432 | 00:41:29.73 +50:21:54.0 (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) J-Ks=0.150+/-0.026 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:29.89 +50:21:53.2: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:29.89 +50:21:53.2: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 29.89 +50 21 53.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 414748915712338432,2461231.6985,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414748915712338432 20260710.1985 10.93CV 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 10.1985 2461231.6985 11.02 00:46:43.15 +49:55:58.5
122.15284 -12.93169 galactic Cas Second-epoch detections are separated by 5.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414762449154912128 | 00:46:42.86 +49:55:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:43.15 +49:55:58.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:43.15 +49:55:58.5: 13.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 43.15 +49 55 58.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414762449154912128,2461231.6985,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414762449154912128 20260710.1985 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.10 00:41:55.96 +50:06:51.5
121.36995 -12.72861 galactic Cas Second-epoch detections are separated by 7.9" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414744655108673280 | 00:41:55.66 +50:06:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:55.96 +50:06:51.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:55.96 +50:06:51.5: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 55.96 +50 06 51.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414744655108673280,2461231.6985,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414744655108673280 20260710.1985 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.00 00:44:16.75 +50:19:50.6
121.76172 -12.52476 galactic Cas Second-epoch detections are separated by 2.9" 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 | Gaia DR3 414786024234390016 | 00:44:16.65 +50:19:49.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.765+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:16.75 +50:19:50.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:16.75 +50:19:50.6: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 16.75 +50 19 50.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414786024234390016,2461231.6985,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414786024234390016 20260710.1985 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.06 00:43:00.03 +50:33:03.3
121.56035 -12.29836 galactic Cas Second-epoch detections are separated by 6.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414839625425894016 | 00:43:00.04 +50:33:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:00.03 +50:33:03.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:00.03 +50:33:03.3: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 00.03 +50 33 03.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414839625425894016,2461231.6985,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414839625425894016 20260710.1985 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.94 00:34:57.86 +49:17:03.0
120.17044 -13.49923 galactic Cas Second-epoch detections are separated by 3.2" and 5.0 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 391370137413798144 | 00:34:57.67 +49:17:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:57.86 +49:17:03.0: 13.50 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:57.86 +49:17:03.0: 12.85 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 10.1985* 00 34 57.86 +49 17 03.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391370137413798144,2461231.6985,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391370137413798144 20260710.1985 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.00 00:31:58.44 +49:07:28.5
119.65751 -13.62338 galactic Cas Second-epoch detections are separated by 7.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391536816504287360 | 00:31:58.22 +49:07:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.410+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:58.44 +49:07:28.5: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:58.44 +49:07:28.5: 13.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 31 58.44 +49 07 28.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391536816504287360,2461231.6985,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391536816504287360 20260710.1985 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.89 00:33:05.59 +49:06:48.4
119.84454 -13.64830 galactic Cas Second-epoch detections are separated by 3.6" 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 | Gaia DR3 391352575288411008 | 00:33:05.27 +49:06:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:05.59 +49:06:48.4: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:05.59 +49:06:48.4: 13.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 33 05.59 +49 06 48.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391352575288411008,2461231.6985,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391352575288411008 20260710.1985 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.91 00:36:42.33 +49:06:19.3
120.45107 -13.69541 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 | Gaia DR3 391317012959866624 | 00:36:42.01 +49:06:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:42.33 +49:06:19.3: 12.87 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:42.33 +49:06:19.3: 12.81 +/- 0.23 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 10.1985* 00 36 42.33 +49 06 19.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391317012959866624,2461231.6985,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391317012959866624 20260710.1985 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.96 00:44:43.10 +50:10:15.0
121.82911 -12.68653 galactic Cas Second-epoch detections are separated by 3.3" and 5.0 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 414775338355848192 | 00:44:42.89 +50:10:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.537+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:43.10 +50:10:15.0: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:43.10 +50:10:15.0: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 43.10 +50 10 15.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414775338355848192,2461231.6985,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414775338355848192 20260710.1985 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.22 00:30:19.86 +48:50:51.9
119.35783 -13.87747 galactic Cas Second-epoch detections are separated by 4.1" 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 | 00:30:19.86 +48:50:51.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:19.86 +48:50:51.9: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:19.86 +48:50:51.9: 13.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 30 19.86 +48 50 51.9 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.82 00:35:56.60 +48:58:49.7
120.31496 -13.81253 galactic Cas Second-epoch detections are separated by 5.7" and 4.9 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 391356011262256256 | 00:35:56.34 +48:58:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:56.60 +48:58:49.7: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:56.60 +48:58:49.7: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 56.60 +48 58 49.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391356011262256256,2461231.6985,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391356011262256256 20260710.1985 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 10.1985 2461231.6985 11.53 23:33:41.18 +49:58:08.9
110.33754 -10.99171 galactic And Second-epoch detections are separated by 2.1" and 5.0 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 J353.4219+49.9732 | 23:33:43.36 +49:58:40.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 1952CoRut..32....1H BD+49 4154
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:33:41.18 +49:58:08.9: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:33:41.18 +49:58:08.9: 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 10.1985* 23 33 41.18 +49 58 08.9 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.4219+49.9732,2461231.6985,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.4219+49.9732 20260710.1985 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.05 00:35:03.83 +50:12:02.8
120.24845 -12.58564 galactic Cas Second-epoch detections are separated by 1.5" 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 | ATO J008.7639+50.2042 | 00:35:03.71 +50:12:04.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.196+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:03.83 +50:12:02.8: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:03.83 +50:12:02.8: 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 10.1985* 00 35 03.83 +50 12 02.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.7639+50.2042,2461231.6985,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.7639+50.2042 20260710.1985 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.96 00:35:50.04 +48:59:20.0
120.29706 -13.80301 galactic Cas Second-epoch detections are separated by 4.7" 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 | Gaia DR3 391356217420686080 | 00:35:49.75 +48:59:17.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:50.04 +48:59:20.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:50.04 +48:59:20.0: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 50.04 +48 59 20.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391356217420686080,2461231.6985,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391356217420686080 20260710.1985 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.15 00:46:26.92 +51:18:33.0
122.13611 -11.55487 galactic Cas Second-epoch detections are separated by 4.6" and 4.5 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 | 00:46:26.92 +51:18:33.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:26.92 +51:18:33.0: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:26.92 +51:18:33.0: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 26.92 +51 18 33.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.93 00:33:59.40 +50:02:29.6
120.06146 -12.73292 galactic Cas Second-epoch detections are separated by 1.3" 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 | Gaia DR3 391496134574024448 | 00:33:59.43 +50:02:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.767+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:59.40 +50:02:29.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:59.40 +50:02:29.6: 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 10.1985* 00 33 59.40 +50 02 29.6 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391496134574024448,2461231.6985,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391496134574024448 20260710.1985 10.93CV 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 10.1985 2461231.6985 11.60 23:32:20.38 +54:04:39.5
111.39585 -7.01296 galactic Cas Second-epoch detections are separated by 2.1" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1994278183124735616 | 23:32:23.41 +54:04:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5) J-Ks=0.250+/-0.030 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:32:20.38 +54:04:39.5: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:32:20.38 +54:04:39.5: 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 10.1985* 23 32 20.38 +54 04 39.5 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994278183124735616,2461231.6985,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1994278183124735616 20260710.1985 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.10 00:30:06.84 +49:24:56.5
119.37090 -13.30856 galactic Cas Second-epoch detections are separated by 4.9" and 4.9 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 391557153170980352 | 00:30:06.54 +49:24:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:06.84 +49:24:56.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:06.84 +49:24:56.5: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 30 06.84 +49 24 56.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391557153170980352,2461231.6985,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391557153170980352 20260710.1985 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.21 00:42:43.93 +50:52:44.5
121.52835 -11.96899 galactic Cas Second-epoch detections are separated by 4.4" and 4.6 pix
The object was found in VSX10" Gaia DR3 414879512783307648
Type: ROT
# Max. Min./Amp. JD0 Period
12.340 G 12.360 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:43.93 +50:52:44.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:43.93 +50:52:44.5: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 43.93 +50 52 44.5 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 414879512783307648,2461231.6985,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414879512783307648 20260710.1985 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.90 00:38:46.94 +49:15:20.7
120.80824 -13.56381 galactic Cas Second-epoch detections are separated by 5.0" and 4.8 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 391401366116904960 | 00:38:46.73 +49:15:26.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=2.520+/- (Very red!)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:46.94 +49:15:20.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:46.94 +49:15:20.7: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 46.94 +49 15 20.7 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391401366116904960,2461231.6985,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391401366116904960 20260710.1985 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.03 00:46:10.02 +50:39:38.1
122.07733 -12.20242 galactic Cas Second-epoch detections are separated by 4.0" and 5.3 pix
The object was found in VSX 6" Gaia DR3 415181367383938560
Type: VAR
# Max. Min./Amp. JD0 Period
12.450 G 12.470 G 0.061514800000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:10.02 +50:39:38.1: 13.23 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:10.02 +50:39:38.1: 12.69 +/- 0.23 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 10.02 +50 39 38.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415181367383938560,2461231.6985,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415181367383938560 20260710.1985 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.13 00:42:52.48 +50:10:11.2
121.52661 -12.67860 galactic Cas Second-epoch detections are separated by 7.9" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414734244107939712 | 00:42:52.18 +50:10:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:52.48 +50:10:11.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:52.48 +50:10:11.2: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 52.48 +50 10 11.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414734244107939712,2461231.6985,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414734244107939712 20260710.1985 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 10.1985 2461231.6985 11.08 00:39:45.11 +50:27:52.4
121.02853 -12.36400 galactic Cas Second-epoch detections are separated by 5.2" and 4.6 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 415506096972288896 | 00:39:45.09 +50:27:54.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:45.11 +50:27:52.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:45.11 +50:27:52.4: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 39 45.11 +50 27 52.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415506096972288896,2461231.6985,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415506096972288896 20260710.1985 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.19 00:36:50.92 +49:58:17.1
120.52691 -12.83219 galactic Cas Second-epoch detections are separated by 3.9" and 4.8 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 | 00:36:50.92 +49:58:17.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:50.92 +49:58:17.1: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:50.92 +49:58:17.1: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 50.92 +49 58 17.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.04 00:40:09.34 +49:54:02.9
121.06832 -12.93011 galactic Cas Second-epoch detections are separated by 2.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 415459990501821184 | 00:40:09.18 +49:54:02.2 (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) J-Ks=0.233+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:09.34 +49:54:02.9: 13.51 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:09.34 +49:54:02.9: 13.21 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.51 +/- 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 10.1985* 00 40 09.34 +49 54 02.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 415459990501821184,2461231.6985,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415459990501821184 20260710.1985 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.12 00:45:36.48 +50:15:29.1
121.97716 -12.60286 galactic Cas Second-epoch detections are separated by 5.2" and 4.9 pix
The object was found in VSX 7" Gaia DR3 414770802870351744
Type: ROT
# Max. Min./Amp. JD0 Period
14.010 G 14.030 G 4.243590000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:36.48 +50:15:29.1: 12.37 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:36.48 +50:15:29.1: 12.02 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.20 +/- 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 10.1985* 00 45 36.48 +50 15 29.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414770802870351744,2461231.6985,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414770802870351744 20260710.1985 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.10 00:33:35.61 +49:08:21.9
119.93048 -13.62831 galactic Cas Second-epoch detections are separated by 3.8" 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 | Gaia DR3 391353644739414400 | 00:33:35.11 +49:08:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:35.61 +49:08:21.9: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:35.61 +49:08:21.9: 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 10.1985* 00 33 35.61 +49 08 21.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391353644739414400,2461231.6985,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391353644739414400 20260710.1985 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.02 00:43:54.83 +49:43:20.1
121.68332 -13.13126 galactic Cas Second-epoch detections are separated by 3.9" and 5.9 pix
The object was found in VSX23" Gaia DR3 414670816031123200
Type: ROT
# Max. Min./Amp. JD0 Period
14.610 G 14.650 G G
ATTENTION: measured mag 11.02 is 3.6 mag brighter than the VSX record maximum brightness 14.61 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:54.83 +49:43:20.1: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:54.83 +49:43:20.1: 13.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 54.83 +49 43 20.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414670816031123200,2461231.6985,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414670816031123200 20260710.1985 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.10 00:45:25.13 +51:00:06.9
121.96439 -11.85852 galactic Cas Second-epoch detections are separated by 8.5" 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 | 00:45:25.13 +51:00:06.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:25.13 +51:00:06.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:25.13 +51:00:06.9: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 25.13 +51 00 06.9 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.12 00:36:02.94 +49:22:20.1
120.35754 -13.42256 galactic Cas Second-epoch detections are separated by 2.4" and 4.7 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 J009.0105+49.3691 | 00:36:02.94 +49:22:20.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.945+/-0.024 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:02.94 +49:22:20.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:02.94 +49:22:20.1: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 02.94 +49 22 20.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J009.0105+49.3691,2461231.6985,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.0105+49.3691 20260710.1985 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.94 00:34:11.17 +49:07:20.9
120.02878 -13.65201 galactic Cas Second-epoch detections are separated by 2.8" 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 | Gaia DR3 391350067027514112 | 00:34:10.69 +49:07:19.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:11.17 +49:07:20.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:11.17 +49:07:20.9: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 11.17 +49 07 20.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391350067027514112,2461231.6985,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391350067027514112 20260710.1985 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.13 00:46:39.22 +51:36:36.2
122.17462 -11.25466 galactic Cas Second-epoch detections are separated by 2.3" and 4.7 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 415337218858504320 | 00:46:38.99 +51:36:39.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:39.22 +51:36:36.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:39.22 +51:36:36.2: 13.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 39.22 +51 36 36.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415337218858504320,2461231.6985,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415337218858504320 20260710.1985 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 10.1985 2461231.6985 11.21 00:29:47.99 +49:19:48.4
119.31100 -13.38945 galactic Cas Second-epoch detections are separated by 5.3" and 4.8 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 391555164604379008 | 00:29:47.99 +49:19:48.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.272+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:47.99 +49:19:48.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:47.99 +49:19:48.4: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 29 47.99 +49 19 48.4 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 391555164604379008,2461231.6985,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391555164604379008 20260710.1985 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.13 00:35:06.30 +49:53:43.8
120.23485 -12.89070 galactic Cas Second-epoch detections are separated by 2.1" and 5.0 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 391490637016164352 | 00:35:05.96 +49:53:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:06.30 +49:53:43.8: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:06.30 +49:53:43.8: 13.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 06.30 +49 53 43.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391490637016164352,2461231.6985,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391490637016164352 20260710.1985 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 10.1985 2461231.6985 11.05 00:40:28.12 +50:15:58.0
121.13633 -12.56739 galactic Cas Second-epoch detections are separated by 0.7" 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 | Gaia DR3 415495037436884352 | 00:40:28.02 +50:15:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.679+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:28.12 +50:15:58.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:28.12 +50:15:58.0: 12.59 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 10.1985* 00 40 28.12 +50 15 58.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415495037436884352,2461231.6985,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415495037436884352 20260710.1985 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.27 00:36:12.15 +49:57:42.5
120.41994 -12.83562 galactic Cas Second-epoch detections are separated by 4.7" and 4.7 pix
The object was found in VSX14" Gaia DR3 391500807498712320
Type: ROT
# Max. Min./Amp. JD0 Period
16.660 G 16.710 G K
ATTENTION: measured mag 11.27 is 5.4 mag brighter than the VSX record maximum brightness 16.66 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:12.15 +49:57:42.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:12.15 +49:57:42.5: 13.33 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 36 12.15 +49 57 42.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391500807498712320,2461231.6985,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391500807498712320 20260710.1985 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.74 23:33:31.05 +52:42:15.6
111.14674 -8.37526 galactic Cas Second-epoch detections are separated by 5.5" 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 J353.3771+52.7070 | 23:33:31.05 +52:42:15.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:33:31.05 +52:42:15.6: 13.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:33:31.05 +52:42:15.6: 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 10.1985* 23 33 31.05 +52 42 15.6 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.3771+52.7070,2461231.6985,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J353.3771+52.7070 20260710.1985 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 10.1985 2461231.6985 11.13 00:33:31.39 +50:04:38.4
119.98742 -12.69197 galactic Cas Second-epoch detections are separated by 3.2" and 4.7 pix
The object was found in VSX20" Gaia DR3 391684013623963648
Type: ROT
# Max. Min./Amp. JD0 Period
17.070 G 17.160 G 5.698800000000 K
ATTENTION: measured mag 11.13 is 5.9 mag brighter than the VSX record maximum brightness 17.07 - 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:31.39 +50:04:38.4: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:31.39 +50:04:38.4: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 33 31.39 +50 04 38.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391684013623963648,2461231.6985,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391684013623963648 20260710.1985 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 10.1985 2461231.6985 11.24 00:41:50.21 +50:26:18.5
121.36689 -12.40410 galactic Cas Second-epoch detections are separated by 5.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414843228899772544 | 00:41:50.23 +50:26:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.340+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:50.21 +50:26:18.5: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:50.21 +50:26:18.5: 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 10.1985* 00 41 50.21 +50 26 18.5 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 414843228899772544,2461231.6985,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414843228899772544 20260710.1985 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.16 00:28:14.13 +48:45:48.1
118.99609 -13.93099 galactic Cas Second-epoch detections are separated by 4.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391185247661419520 | 00:28:13.88 +48:45:47.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:14.13 +48:45:48.1: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:14.13 +48:45:48.1: 13.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 28 14.13 +48 45 48.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391185247661419520,2461231.6985,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391185247661419520 20260710.1985 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.01 00:40:03.09 +48:49:47.8
121.00108 -13.99911 galactic Cas Second-epoch detections are separated by 4.7" 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 | Gaia DR3 390635938524236800 | 00:40:02.51 +48:49:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:03.09 +48:49:47.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:03.09 +48:49:47.8: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 40 03.09 +48 49 47.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390635938524236800,2461231.6985,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390635938524236800 20260710.1985 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.91 00:44:45.05 +49:44:26.1
121.82268 -13.11676 galactic Cas Second-epoch detections are separated by 5.7" 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 | Gaia DR3 414674492523401344 | 00:44:44.62 +49:44:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:45.05 +49:44:26.1: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:45.05 +49:44:26.1: 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 10.1985* 00 44 45.05 +49 44 26.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414674492523401344,2461231.6985,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414674492523401344 20260710.1985 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.12 00:37:58.58 +49:59:06.2
120.71333 -12.82870 galactic Cas Second-epoch detections are separated by 3.1" and 4.9 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 J009.4982+49.9809 | 00:37:58.58 +49:59:06.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:58.58 +49:59:06.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:58.58 +49:59:06.2: 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 10.1985* 00 37 58.58 +49 59 06.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J009.4982+49.9809,2461231.6985,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J009.4982+49.9809 20260710.1985 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.38 00:46:09.87 +51:24:24.0
122.09287 -11.45649 galactic Cas Second-epoch detections are separated by 6.0" and 5.7 pix
The object was found in VSX 6" Gaia DR3 415239126104182656
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.680 G 12.700 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:09.87 +51:24:24.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:09.87 +51:24:24.0: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 46 09.87 +51 24 24.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415239126104182656,2461231.6985,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415239126104182656 20260710.1985 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.14 00:42:09.50 +50:18:51.6
121.41458 -12.53007 galactic Cas Second-epoch detections are separated by 6.8" and 4.8 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 414841446492098560 | 00:42:09.37 +50:18:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.294+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:09.50 +50:18:51.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:09.50 +50:18:51.6: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 09.50 +50 18 51.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414841446492098560,2461231.6985,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414841446492098560 20260710.1985 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.06 00:41:07.40 +50:43:02.2
121.26235 -12.12103 galactic Cas Second-epoch detections are separated by 5.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414856457398868096 | 00:41:07.32 +50:43:03.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:07.40 +50:43:02.2: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:07.40 +50:43:02.2: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 07.40 +50 43 02.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414856457398868096,2461231.6985,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414856457398868096 20260710.1985 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.12 00:35:22.89 +49:14:54.1
120.23789 -13.53938 galactic Cas Second-epoch detections are separated by 1.8" 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 J008.8339+49.2509 | 00:35:22.88 +49:14:56.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:22.89 +49:14:54.1: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:22.89 +49:14:54.1: 13.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 35 22.89 +49 14 54.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.8339+49.2509,2461231.6985,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.8339+49.2509 20260710.1985 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.10 00:31:28.00 +49:10:51.3
119.57699 -13.56069 galactic Cas Second-epoch detections are separated by 6.3" 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 | Gaia DR3 391538152235341952 | 00:31:27.50 +49:10:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:28.00 +49:10:51.3: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:28.00 +49:10:51.3: 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 10.1985* 00 31 28.00 +49 10 51.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391538152235341952,2461231.6985,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391538152235341952 20260710.1985 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.30 00:38:26.44 +50:13:43.8
120.80270 -12.58917 galactic Cas Second-epoch detections are separated by 3.1" and 4.8 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 | 00:38:26.44 +50:13:43.8 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.027 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:26.44 +50:13:43.8: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:26.44 +50:13:43.8: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 26.44 +50 13 43.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.14 00:33:11.13 +49:10:15.8
119.86436 -13.59195 galactic Cas Second-epoch detections are separated by 3.3" 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 | Gaia DR3 391353228123439616 | 00:33:10.98 +49:10:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.732+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:11.13 +49:10:15.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:11.13 +49:10:15.8: 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 10.1985* 00 33 11.13 +49 10 15.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391353228123439616,2461231.6985,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391353228123439616 20260710.1985 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.25 00:43:40.88 +49:57:32.0
121.65226 -12.89359 galactic Cas Second-epoch detections are separated by 3.2" and 5.0 pix
The object was found in VSX 5" Gaia DR3 414680638617037184
Type: ROT
# Max. Min./Amp. JD0 Period
12.540 G 12.570 G 20.274000000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:40.88 +49:57:32.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:40.88 +49:57:32.0: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 40.88 +49 57 32.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414680638617037184,2461231.6985,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414680638617037184 20260710.1985 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.23 00:45:01.41 +50:21:07.3
121.88392 -12.50667 galactic Cas Second-epoch detections are separated by 4.3" and 4.8 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 J011.2502+50.3506 | 00:45:01.41 +50:21:07.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.346+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:01.41 +50:21:07.3: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:01.41 +50:21:07.3: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 01.41 +50 21 07.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J011.2502+50.3506,2461231.6985,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.2502+50.3506 20260710.1985 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.24 00:36:24.46 +50:09:02.1
120.46529 -12.64917 galactic Cas Second-epoch detections are separated by 6.0" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391509569231931904 | 00:36:24.19 +50:09:03.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:24.46 +50:09:02.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:24.46 +50:09:02.1: 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 10.1985* 00 36 24.46 +50 09 02.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391509569231931904,2461231.6985,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391509569231931904 20260710.1985 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.20 00:45:08.56 +50:23:58.5
121.90460 -12.45961 galactic Cas Second-epoch detections are separated by 2.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 414807494771897728 | 00:45:08.26 +50:23:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:08.56 +50:23:58.5: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:08.56 +50:23:58.5: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 08.56 +50 23 58.5 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 414807494771897728,2461231.6985,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414807494771897728 20260710.1985 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.90 23:38:36.59 +57:11:43.8
113.15845 -4.28782 galactic Cas Second-epoch detections are separated by 4.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1998643106852477184 | 23:38:38.98 +57:12:18.0 (Gaia DR3) | DSCT/GDOR (local) | 2.310740000000 (local) | Gaia3var=VARIABLE SpType: A2V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:38:36.59 +57:11:43.8: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:38:36.59 +57:11:43.8: 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 10.1985* 23 38 36.59 +57 11 43.8 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 1998643106852477184,2461231.6985,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1998643106852477184 20260710.1985 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 10.1985 2461231.6985 11.23 00:44:37.90 +50:16:26.2
121.81775 -12.58308 galactic Cas Second-epoch detections are separated by 8.2" and 4.3 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 | 00:44:37.90 +50:16:26.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:37.90 +50:16:26.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:37.90 +50:16:26.2: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 37.90 +50 16 26.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.14 00:34:04.89 +49:39:52.6
120.04977 -13.10998 galactic Cas Second-epoch detections are separated by 5.0" and 5.0 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 391483863849544192 | 00:34:04.61 +49:39:54.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:04.89 +49:39:52.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:04.89 +49:39:52.6: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 34 04.89 +49 39 52.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391483863849544192,2461231.6985,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391483863849544192 20260710.1985 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.27 00:45:43.06 +51:24:41.2
122.02190 -11.45020 galactic Cas Second-epoch detections are separated by 2.5" 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 | Gaia DR3 415241943602724864 | 00:45:42.74 +51:24:41.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:43.06 +51:24:41.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:43.06 +51:24:41.2: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 43.06 +51 24 41.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415241943602724864,2461231.6985,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415241943602724864 20260710.1985 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.07 00:42:00.00 +49:31:12.7
121.35807 -13.32271 galactic Cas Second-epoch detections are separated by 3.1" 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 | ATO J010.5066+49.5215 | 00:41:59.75 +49:31:13.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:00.00 +49:31:12.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:00.00 +49:31:12.7: 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 10.1985* 00 42 00.00 +49 31 12.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.5066+49.5215,2461231.6985,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.5066+49.5215 20260710.1985 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 12.02 23:25:30.77 +57:09:53.7
111.45383 -3.77954 galactic Cas Second-epoch detections are separated by 4.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:25:30.77 +57:09:53.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:25:30.77 +57:09:53.7: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:25:30.77 +57:09:53.7: 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 10.1985* 23 25 30.77 +57 09 53.7 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,2461231.6985,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 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 10.1985 2461231.6985 11.30 00:34:44.60 +49:41:17.9
120.16109 -13.09361 galactic Cas Second-epoch detections are separated by 2.2" and 5.0 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 J008.6815+49.6903 | 00:34:44.60 +49:41:17.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.635+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:44.60 +49:41:17.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:44.60 +49:41:17.9: 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 10.1985* 00 34 44.60 +49 41 17.9 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J008.6815+49.6903,2461231.6985,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J008.6815+49.6903 20260710.1985 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.26 00:30:19.81 +48:56:58.7
119.36654 -13.77593 galactic Cas Second-epoch detections are separated by 6.6" and 4.8 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 391166036268846080 | 00:30:19.50 +48:56:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:19.81 +48:56:58.7: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:19.81 +48:56:58.7: 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 10.1985* 00 30 19.81 +48 56 58.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391166036268846080,2461231.6985,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391166036268846080 20260710.1985 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 12.16 23:24:32.34 +57:07:12.4
111.31405 -3.77849 galactic Cas Second-epoch detections are separated by 0.6" and 4.4 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 J351.1461+57.1134 | 23:24:37.14 +57:07:10.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B6 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:24:32.34 +57:07:12.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:24:32.34 +57:07:12.4: 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 10.1985* 23 24 32.34 +57 07 12.4 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.1461+57.1134,2461231.6985,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.1461+57.1134 20260710.1985 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 10.1985 2461231.6985 11.27 00:39:21.14 +50:28:23.6
120.96394 -12.35234 galactic Cas Second-epoch detections are separated by 6.1" and 6.1 pix
The object was found in VSX 4" Gaia DR3 415506754105494144
Type: ROT
# Max. Min./Amp. JD0 Period
12.690 G 12.710 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:21.14 +50:28:23.6: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:21.14 +50:28:23.6: 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 10.1985* 00 39 21.14 +50 28 23.6 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 415506754105494144,2461231.6985,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415506754105494144 20260710.1985 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.38 00:45:50.71 +50:35:01.8
122.02341 -12.27805 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 | 00:45:50.71 +50:35:01.8 (user input) | T | P | (position from user input) J-Ks=0.932+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:50.71 +50:35:01.8: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:50.71 +50:35:01.8: 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 10.1985* 00 45 50.71 +50 35 01.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.29 00:41:27.08 +50:23:44.8
121.30236 -12.44437 galactic Cas Second-epoch detections are separated by 5.2" 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 | 00:41:27.08 +50:23:44.8 (user input) | T | P | (position from user input) J-Ks=0.256+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:27.08 +50:23:44.8: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:27.08 +50:23:44.8: 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 10.1985* 00 41 27.08 +50 23 44.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.12 00:40:29.75 +49:05:50.1
121.08841 -13.73533 galactic Cas Second-epoch detections are separated by 6.8" and 5.0 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 390646658762523648 | 00:40:29.25 +49:05:50.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:40:29.75 +49:05:50.1: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:40:29.75 +49:05:50.1: 13.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 40 29.75 +49 05 50.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390646658762523648,2461231.6985,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 390646658762523648 20260710.1985 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.43 00:43:25.12 +50:19:24.6
121.62087 -12.52783 galactic Cas Second-epoch detections are separated by 7.1" and 4.5 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 | 00:43:25.12 +50:19:24.6 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.028 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:25.12 +50:19:24.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:25.12 +50:19:24.6: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 43 25.12 +50 19 24.6 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.29 00:41:25.86 +49:49:30.6
121.27574 -13.01440 galactic Cas 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 | Gaia DR3 414710428510211712 | 00:41:25.52 +49:49:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:41:25.86 +49:49:30.6: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:41:25.86 +49:49:30.6: 13.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 41 25.86 +49 49 30.6 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 414710428510211712,2461231.6985,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414710428510211712 20260710.1985 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.21 00:42:02.89 +49:45:10.8
121.37506 -13.09036 galactic Cas Second-epoch detections are separated by 4.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J010.5168+49.7520 | 00:42:02.64 +49:45:12.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:42:02.89 +49:45:10.8: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:42:02.89 +49:45:10.8: 13.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 42 02.89 +49 45 10.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J010.5168+49.7520,2461231.6985,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J010.5168+49.7520 20260710.1985 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.20 00:33:40.47 +49:11:41.2
119.94811 -13.57403 galactic Cas Second-epoch detections are separated by 8.6" and 4.3 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 | 00:33:40.47 +49:11:41.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:40.47 +49:11:41.2: 13.16 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:40.47 +49:11:41.2: 12.77 +/- 0.21 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 33 40.47 +49 11 41.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.30 00:36:35.35 +49:51:39.6
120.47749 -12.93997 galactic Cas Second-epoch detections are separated by 4.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:36:35.35 +49:51:39.6 (user input) | T | P | (position from user input) J-Ks=0.309+/-0.027 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:36:35.35 +49:51:39.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:36:35.35 +49:51:39.6: 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 10.1985* 00 36 35.35 +49 51 39.6 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
target,2461231.6985,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.31 00:48:02.49 +51:33:32.7
122.39358 -11.30912 galactic Cas Second-epoch detections are separated by 4.6" 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 | 00:48:02.49 +51:33:32.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:02.49 +51:33:32.7: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:02.49 +51:33:32.7: 13.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 48 02.49 +51 33 32.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 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 10.1985 2461231.6985 11.24 00:47:02.28 +50:32:18.5
122.21634 -12.32716 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 | target | 00:47:02.28 +50:32:18.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:02.28 +50:32:18.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:02.28 +50:32:18.5: 13.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 47 02.28 +50 32 18.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.33 00:38:35.35 +48:55:17.9
120.75820 -13.89587 galactic Cas Second-epoch detections are separated by 3.7" 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 | 00:38:35.35 +48:55:17.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:35.35 +48:55:17.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:35.35 +48:55:17.9: 13.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 38 35.35 +48 55 17.9 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.32 00:38:29.97 +50:26:20.4
120.82340 -12.37977 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 | Gaia DR3 415511667548082688 | 00:38:29.82 +50:26:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.335+/-0.026 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:38:29.97 +50:26:20.4: 12.54 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:38:29.97 +50:26:20.4: 12.65 +/- 0.21 detection
Forced photometry reference-image weighted average: 12.57 +/- 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 10.1985* 00 38 29.97 +50 26 20.4 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415511667548082688,2461231.6985,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415511667548082688 20260710.1985 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.28 00:28:30.56 +49:04:19.4
119.07147 -13.62775 galactic Cas Second-epoch detections are separated by 5.5" and 4.9 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 | 00:28:30.56 +49:04:19.4 (user input) | T | P | (position from user input) J-Ks=0.272+/-0.029 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:30.56 +49:04:19.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:30.56 +49:04:19.4: 13.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 28 30.56 +49 04 19.4 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.60 00:12:08.83 +50:38:18.1
116.58710 -11.74872 galactic Cas Second-epoch detections are separated by 2.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 395243338924336128 | 00:12:12.52 +50:37:59.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:12:08.83 +50:38:18.1: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:12:08.83 +50:38:18.1: 13.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 12 08.83 +50 38 18.1 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395243338924336128,2461231.6985,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 395243338924336128 20260710.1985 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.39 00:29:50.13 +48:49:10.3
119.27166 -13.89863 galactic Cas Second-epoch detections are separated by 5.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 391142980884409600 | 00:29:49.95 +48:49:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.996+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:50.13 +48:49:10.3: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:50.13 +48:49:10.3: 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 10.1985* 00 29 50.13 +48 49 10.3 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391142980884409600,2461231.6985,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 391142980884409600 20260710.1985 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.43 00:30:50.84 +49:58:09.9
119.53963 -12.76666 galactic Cas Second-epoch detections are separated by 3.8" 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 | target | 00:30:50.84 +49:58:09.9 (user input) | T | P | (position from user input) J-Ks=0.024+/-0.031 (A)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:50.84 +49:58:09.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:50.84 +49:58:09.9: 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 10.1985* 00 30 50.84 +49 58 09.9 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.36 00:45:56.19 +51:22:51.1
122.05602 -11.48153 galactic Cas Second-epoch detections are separated by 4.7" 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 | Large-amplitude variable Gaia DR2 415241600001840512 | 00:45:56.19 +51:22:51.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.441+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:56.19 +51:22:51.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:56.19 +51:22:51.1: 13.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 45 56.19 +51 22 51.1 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 415241600001840512,2461231.6985,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415241600001840512 20260710.1985 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.46 00:43:44.44 +51:06:54.1
121.69825 -11.73828 galactic Cas Second-epoch detections are separated by 6.5" and 4.7 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 | 00:43:44.44 +51:06:54.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:43:44.44 +51:06:54.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:43:44.44 +51:06:54.1: 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 10.1985* 00 43 44.44 +51 06 54.1 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,2461231.6985,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.07 00:55:31.18 +56:33:11.6
123.49776 -6.31404 galactic Cas Second-epoch detections are separated by 2.5" and 4.8 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 | 00:55:31.18 +56:33:11.6 (user input) | T | P | (position from user input) J-Ks=0.253+/-0.032 (F)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:55:31.18 +56:33:11.6: 12.27 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:55:31.18 +56:33:11.6: 12.39 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.31 +/- 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 10.1985* 00 55 31.18 +56 33 11.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.60 23:57:50.00 +56:34:46.4
115.56356 -5.52337 galactic Cas Second-epoch detections are separated by 0.7" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J359.4535+56.5833 | 23:57:50.00 +56:34:46.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:57:50.00 +56:34:46.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:57:50.00 +56:34:46.4: 13.22 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 10.1985* 23 57 50.00 +56 34 46.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.4535+56.5833,2461231.6985,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J359.4535+56.5833 20260710.1985 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 11.13 00:53:12.38 +54:48:07.2
123.18929 -8.06887 galactic Cas Second-epoch detections are separated by 3.6" and 5.0 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 | 00:53:12.38 +54:48:07.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:53:12.38 +54:48:07.2: 13.23 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:53:12.38 +54:48:07.2: 13.21 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.23 +/- 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 10.1985* 00 53 12.38 +54 48 07.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461231.6985,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.1985 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 10.1985 2461231.6985 10.91 00:44:39.41 +51:41:05.1
121.86066 -11.17289 galactic Cas Second-epoch detections are separated by 2.1" and 4.9 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 415293753790831232 | 00:44:39.26 +51:41:07.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:39.41 +51:41:05.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:39.41 +51:41:05.1: 13.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 44 39.41 +51 41 05.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415293753790831232,2461231.6985,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 415293753790831232 20260710.1985 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1985 2461231.6985 10.81 00:48:55.16 +53:00:35.8
122.54740 -9.85992 galactic Cas Second-epoch detections are separated by 2.4" and 5.0 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 417011053513598336 | 00:48:54.96 +53:00:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.402+/-0.027 (G)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:55.16 +53:00:35.8: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:55.16 +53:00:35.8: 13.18 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.1985* 00 48 55.16 +53 00 35.8 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 417011053513598336,2461231.6985,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 417011053513598336 20260710.1985 10.81CV 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
## 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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461231.69888341 10.07.2026 04:46:13.527 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 195
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.84
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: 8 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): 22553
Objects passed selection criteria: 22501
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 18272.2
Average stars matched: 17722.5 (96.9913 %)
Memory usage VmPeak: 126216 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 9 23:58:26 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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Last image: 2461231.69888341 10.07.2026 04:46:13.527 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1080
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
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: 345 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): 155209
Objects passed selection criteria: 154777
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 129382
Average stars matched: 124578 (96.2869 %)
Memory usage VmPeak: 2044720 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 00:31:23 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
SExtractor catalog cache: saved Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461231.69821250
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits exists and is non-empty
Saving wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits to local_wcs_cache/
'wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'local_wcs_cache/wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits'
wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits exists and is non-empty
Saving wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits to local_wcs_cache/
'wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'local_wcs_cache/wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits'
wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits'
wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
Image size: 942.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:57.833 +53:58:30.83 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 23:59:57.833 +53:58:30.83
Angular distance between the image centers 0.0325 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
Image size: 944.1'x628.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 00:00:01.516 +53:58:52.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.466 +54:00:23.28
Second-epoch image center 00:00:01.516 +53:58:52.90
Angular distance between the image centers 0.0251 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 23:59:57.833 +53:58:30.83
Second-epoch second image center 00:00:01.516 +53:58:52.90
Angular distance between the image centers 0.01091 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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits &> /tmp/tmp.eD6OHIZwLV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits &> /tmp/tmp.dZGxMazz1K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits &> /tmp/tmp.XtdV5dMFyk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits &> /tmp/tmp.990VdWr5Q2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits and wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q1b1x1_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 22.497200
a=0.000000 b=1.000000 c=22.497200
From vast_summary.log: estimated ref. image limiting mag.: -7.84
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.66
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.66
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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits (aperture=6.5)
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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 173 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
2.9 pix fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
2.9 pix fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
2.3 pix wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
2.4 pix wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Limiting magnitude estimates:
14.7 mag. Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
14.7 mag. Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
13.9 mag. fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
14.0 mag. fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.3 (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.eD6OHIZwLV (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=0, passed=23386
Got 23386 stars (including 21456 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_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 345 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 237 matched stars entering correct_measured_positions(), 165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 5401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.13"
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 345.0050 through 0 to 14.8900, gap 14.8900 to 345.0050
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 391 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 311 matched stars entering correct_measured_positions(), 5436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.00"
Accuracy estimation diagnostic: 307 matched stars entering correct_measured_positions(), 6969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.20"
Excluding outliers - 307 stars left (next iteration limit 248)
WCS_QUALITY_DIAG: file=Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits N_match=307 sigma_overall_arcsec=9.990 sigma_q1_arcsec=26.120 sigma_q2_arcsec=23.868 sigma_q3_arcsec=5.575 sigma_q4_arcsec=9.476 n_q1=31 n_q2=24 n_q3=81 n_q4=171 worst_quadrant_to_overall_ratio=2.615
The image catalog is written to wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits -region wcs_Cas-04-Q1b1x1_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-Q1b1x1_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.dZGxMazz1K (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=0, passed=23366
Got 23366 stars (including 21472 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_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 349 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(), 166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.90"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 228 matched stars entering correct_measured_positions(), 5186 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.88"
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 345.0155 through 0 to 14.8915, gap 14.8915 to 345.0155
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 391 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 316 matched stars entering correct_measured_positions(), 5214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.84"
Accuracy estimation diagnostic: 313 matched stars entering correct_measured_positions(), 6885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.49"
Excluding outliers - 313 stars left (next iteration limit 250)
WCS_QUALITY_DIAG: file=Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits N_match=313 sigma_overall_arcsec=12.138 sigma_q1_arcsec=31.673 sigma_q2_arcsec=30.888 sigma_q3_arcsec=5.656 sigma_q4_arcsec=10.621 n_q1=29 n_q2=29 n_q3=87 n_q4=168 worst_quadrant_to_overall_ratio=2.609
The image catalog is written to wcs_Cas-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits -region wcs_Cas-04-Q1b1x1_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-Q1b1x1_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.XtdV5dMFyk (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_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.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_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=619, bad_region=0, passed=13159
Got 13159 stars (including 12523 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits.wcscat
util/solve_plate_with_UCAC5 got 13159 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.8'
Seting catalog search parameters based on the expected field of view 942.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013094 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010476 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3943 through 0 to 15.3861, gap 15.3861 to 345.3943
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 12677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 345.3943 through 0 to 15.3865, gap 15.3865 to 345.3943
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 12677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 12667 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 970 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits N_match=970 sigma_overall_arcsec=0.441 sigma_q1_arcsec=0.480 sigma_q2_arcsec=0.534 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.427 n_q1=273 n_q2=154 n_q3=309 n_q4=234 worst_quadrant_to_overall_ratio=1.211
The image catalog is written to wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits -region wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.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.990VdWr5Q2 (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_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.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_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=691, bad_region=0, passed=13590
Got 13590 stars (including 12885 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat
util/solve_plate_with_UCAC5 got 13590 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.1'
Seting catalog search parameters based on the expected field of view 944.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013113 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010490 (37.8 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 345.3486 through 0 to 15.4159, gap 15.4159 to 345.3486
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 12625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.25"
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 345.3528 through 0 to 15.4216, gap 15.4216 to 345.3528
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 12632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.17"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 12805 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.12"
Excluding outliers - 946 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits N_match=946 sigma_overall_arcsec=1.548 sigma_q1_arcsec=1.265 sigma_q2_arcsec=1.163 sigma_q3_arcsec=1.199 sigma_q4_arcsec=1.327 n_q1=259 n_q2=165 n_q3=286 n_q4=236 worst_quadrant_to_overall_ratio=0.857
The image catalog is written to wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits -region wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.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-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits sigma_overall=9.990 worst_q_ratio=2.615
ref2=Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits sigma_overall=12.138 worst_q_ratio=2.609
new1=fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits sigma_overall=0.441 worst_q_ratio=1.211
new2=fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits sigma_overall=1.548 worst_q_ratio=0.857
reference average sigma_overall=11.064 worst_q_ratio=2.612
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006_astrometric_residuals.png (307 matched stars from wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 6.11 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007_astrometric_residuals.png (313 matched stars from wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 5.59 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122_astrometric_residuals.png (970 matched stars from wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123_astrometric_residuals.png (946 matched stars from wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.94 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-45-15_20.00sec_-0.00C_LIGHTs_0122.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Cas-04-Q1b1x1_235012_TTUQ1b1x1_2454513_CXxEnEIg/wcs_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123.fits'
Preparing the HTML report for the field Cas-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:09.93 +49:02:17.0: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:06.15 +48:42:26.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:09.93 +49:02:17.0: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:23.57 +49:19:33.0: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:54:39.08 +54:50:43.1: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:48.38 +48:44:52.3: 13.54 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:06.15 +48:42:26.2: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 00:28:06.15 +48:42:26.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:23.57 +49:19:33.0: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:54:39.08 +54:50:43.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 00:54:39.08 +54:50:43.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:29:36.73 +48:43:49.9: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:48.38 +48:44:52.3: 14.54 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.09
Forced photometry filter KEPT candidate at 00:27:48.38 +48:44:52.3: ref_mag=13.69 +/- 0.09 new_mean_mag=9.7240 delta=3.97 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:29:36.73 +48:43:49.9: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:46:53.36 +50:47:03.4: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:15.80 +49:05:57.8: 15.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:46:53.36 +50:47:03.4: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:15.80 +49:05:57.8: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:46.84 +50:46:19.3: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:29.49 +49:19:02.2: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:46.84 +50:46:19.3: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:29.49 +49:19:02.2: 15.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:30.22 +49:04:17.1: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:30.22 +49:04:17.1: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:37:47.79 +49:14:14.2: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:37:47.79 +49:14:14.2: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:30.75 +49:44:36.9: 15.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:30.75 +49:44:36.9: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:11:31.33 +56:01:29.3: 14.81 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:11:31.33 +56:01:29.3: 14.70 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.19
Forced photometry filter KEPT candidate at 23:11:31.33 +56:01:29.3: ref_mag=14.75 +/- 0.19 new_mean_mag=11.1866 delta=3.56 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:44:04.93 +49:03:55.9: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:44:04.93 +49:03:55.9: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:30:23.39 +48:54:32.5: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:32:51.85 +49:19:38.8: 15.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:30:23.39 +48:54:32.5: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:48:02.30 +50:47:44.6: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:32:51.85 +49:19:38.8: 15.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:48:02.30 +50:47:44.6: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:27:08.02 +48:44:41.6: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:32:49.72 +49:11:25.7: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:27:08.02 +48:44:41.6: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:27.46 +50:43:41.0: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:35:09.45 +49:16:34.4: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:32:49.72 +49:11:25.7: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:27.46 +50:43:41.0: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:35:09.45 +49:16:34.4: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:39:35.16 +48:51:40.5: 13.33 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:39:35.16 +48:51:40.5: 13.46 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.06
Forced photometry filter KEPT candidate at 00:39:35.16 +48:51:40.5: ref_mag=13.38 +/- 0.06 new_mean_mag=10.6841 delta=2.70 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:36:42.81 +52:12:23.4: 15.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:36:42.81 +52:12:23.4: 15.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:10:51.78 +54:50:07.5: 14.61 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:10:51.78 +54:50:07.5: 14.42 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.14
Forced photometry filter KEPT candidate at 23:10:51.78 +54:50:07.5: ref_mag=14.50 +/- 0.14 new_mean_mag=11.6763 delta=2.83 (need > 0.90)
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:01.04 +49:25:53.0: 15.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:01.04 +49:25:53.0: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:47:48.52 +50:46:25.5: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:47:48.52 +50:46:25.5: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:33:37.46 +49:04:29.0: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:33:37.46 +49:04:29.0: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:40.16 +48:54:44.3: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:40.16 +48:54:44.3: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:31:09.43 +54:16:19.7: 15.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:45:56.32 +51:07:56.6: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:31:09.43 +54:16:19.7: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:45:56.32 +51:07:56.6: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 23:16:48.80 +55:26:59.8: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 23:16:48.80 +55:26:59.8: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:32.63 +48:57:00.3: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:31:24.77 +49:05:00.4: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:32.63 +48:57:00.3: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:31:24.77 +49:05:00.4: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:28:48.49 +48:40:23.3: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:28:48.49 +48:40:23.3: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 00:28:48.49 +48:40:23.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-08-38_20.00sec_4.90C_LIGHT_0006.fits at 00:34:57.81 +49:53:58.7: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q1b1x1_2026-06-15_03-09-29_20.00sec_5.00C_LIGHT_0007.fits at 00:34:57.81 +49:53:58.7: 15.03 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out31547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32093.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 1095s
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: 35s
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Considering the candidate 31425_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31425_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:09.70 +49:21:15.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31435_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31435_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:48.71 +49:01:18.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31436_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31436_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:58.44 +51:26:42.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31438_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31438_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31439_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31439_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:45.36 +48:57:10.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31449_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31449_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:34.69 +49:34:22.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31451_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31451_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:42.56 +49:49:59.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31454_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31454_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31458_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31458_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:09.38 +49:58:03.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31463_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31463_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31466_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31466_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:56.01 +49:20:55.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31470_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31470_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:26.85 +49:53:40.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31480_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31480_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:50.99 +49:50:46.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31485_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31485_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:15.39 +49:44:52.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31487_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31487_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:28.17 +50:24:36.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31489_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31489_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:11.51 +50:39:12.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31497_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31497_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:39.70 +50:41:41.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31506_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31506_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31513_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31513_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:31.34 +49:33:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31515_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31515_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:37.60 +50:29:03.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31516_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31516_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:43.77 +48:49:43.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31537_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31537_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:46.53 +50:16:12.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31539_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31539_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:55.83 +50:17:22.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31547_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31547_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31553_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31553_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31555_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31555_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31558_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31558_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:56.17 +49:37:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31560_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31560_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31562_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31562_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:08.10 +51:42:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31566_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31566_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 31567_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31567_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:54.28 +50:30:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31574_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31574_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:24.62 +49:35:30.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31576_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31576_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:56.94 +49:24:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31587_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31587_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31599_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31599_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31600_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31600_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 31603_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31603_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31604_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31604_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:40.10 +49:34:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31608_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31608_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:20.29 +49:36:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31609_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31609_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:14.48 +50:00:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31611_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31611_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:31.92 +50:22:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31612_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31612_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31619_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31619_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:00.34 +50:06:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31623_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31623_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:41.48 +49:37:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31626_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31626_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:50.85 +50:22:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31629_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31629_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31640_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31640_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:45.94 +49:22:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31650_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31650_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:23.60 +50:04:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31651_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31651_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31656_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31656_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:12.50 +50:26:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31662_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31662_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:58.25 +49:52:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31667_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31667_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:15.06 +50:07:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31672_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31672_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 31683_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31683_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:11.81 +49:53:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31688_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31688_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:28.33 +49:30:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31691_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31691_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31692_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31692_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31693_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31693_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:47.69 +51:06:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31696_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31696_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:08.07 +49:26:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31697_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31697_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:56.82 +48:55:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31705_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31705_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:50.23 +49:42:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31710_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31710_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31714_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31714_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:26.27 +50:06:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31715_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31715_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31718_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31718_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:51.32 +49:49:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31721_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31721_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:13.95 +49:12:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31722_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31722_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31727_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31727_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:24.17 +50:56:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31730_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31730_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:22.71 +49:20:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31737_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31737_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31738_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31738_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31739_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31739_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31741_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31741_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:23.96 +49:40:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31743_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31743_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:31.39 +49:59:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31746_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31746_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:34.23 +50:17:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31747_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31747_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:24.80 +50:55:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31749_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31749_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:14.80 +49:18:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31753_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31753_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:19.20 +50:11:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31756_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31756_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:59.29 +49:31:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31759_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31759_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31761_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31761_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:23.02 +49:46:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31764_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31764_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:10.75 +50:37:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31773_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31773_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31774_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31774_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31776_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31776_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:42.89 +49:24:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31779_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31779_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:03.21 +49:14:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31780_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31780_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:49.13 +50:22:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31786_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31786_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:12.71 +49:28:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31796_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31796_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:11.61 +49:08:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31822_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31822_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:26.10 +49:32:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31823_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31823_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:04.94 +50:22:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31827_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31827_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:27.04 +50:36:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31832_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31832_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:48.70 +49:19:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31837_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31837_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:10.61 +50:33:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31841_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31841_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31848_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31848_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31851_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31851_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:17:58.16 +53:44:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31855_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31855_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:38.80 +49:51:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31858_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31858_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:10.06 +49:39:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31870_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31870_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:31.92 +50:07:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31871_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31871_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:16.49 +49:55:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31872_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31872_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31875_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31875_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31879_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31879_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:18.49 +49:41:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31885_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31885_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:28.66 +50:46:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31892_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31892_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:13.18 +50:03:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31904_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31904_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:03.43 +48:45:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31905_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31905_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31906_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31906_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31907_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31907_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:46.03 +48:49:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31908_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31908_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:37.57 +49:38:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31917_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31917_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:50.22 +49:59:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31920_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31920_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:32.53 +50:35:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31921_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31921_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31922_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31922_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31923_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31923_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:11.68 +50:07:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31935_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31935_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:20.43 +51:46:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31937_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31937_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31939_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31939_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31942_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31942_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:24.55 +49:11:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31946_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31946_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:57.98 +50:23:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31949_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31949_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 31959_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31959_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:31.94 +49:05:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31968_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31968_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31977_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31977_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:50.75 +49:48:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31981_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31981_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:23.86 +51:49:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31983_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 31983_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 31985_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31985_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:46:56.31 +58:21:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31991_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31991_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:48:26.77 +51:34:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31993_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31993_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:37.54 +50:13:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31997_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 31997_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:40.62 +49:07:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32000_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32000_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:52.34 +49:24:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32001_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32001_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:30.28 +49:28:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32004_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 32004_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 32010_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32010_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:22.62 +49:43:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32015_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32015_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:43.79 +49:56:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32016_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32016_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:48.04 +50:36:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32018_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 32018_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 32020_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32020_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:26.49 +49:31:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32022_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32022_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:04.10 +50:08:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32025_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 32025_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 32027_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32027_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 32040_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 32040_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 32042_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 32042_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 32046_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32046_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 32050_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32050_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:19.62 +49:50:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32051_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 32051_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 32052_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32052_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 32055_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32055_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 32059_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 32059_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 32063_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 32063_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 32064_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32064_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:17.99 +49:27:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32066_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32066_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:52.95 +49:12:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32068_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32068_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 32069_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32069_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:46.42 +50:08:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32070_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32070_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:56.23 +49:02:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32071_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32071_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:27:26.55 +49:36:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32075_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32075_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 32084_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32084_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:24.09 +48:47:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32086_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32086_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:03.66 +49:44:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32088_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32088_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:14.61 +49:42:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32089_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32089_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:42.37 +50:19:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32093_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 32093_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 32095_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32095_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:22.93 +49:09:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32096_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32096_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 32099_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32099_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:14.00 +49:05:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32102_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 32102_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:21.54 +50:46:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05051_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 05051_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:58:25.07 +51:23:22.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14592_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 14592_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:04:40.80 +55:32:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17508_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 17508_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:44:31.76 +56:34:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17188_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 17188_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:51:53.36 +55:59:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05724_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 05724_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:09:36.66 +51:34:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20884_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 20884_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:12:22.98 +58:01:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191642_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191642_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191645_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191645_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:52:16.34 +57:22:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191653_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191653_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191654_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191654_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 191658_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191658_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191659_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191659_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191663_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191663_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191666_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191666_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:24:48.49 +56:14:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191674_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191674_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 191681_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191681_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:13:00.26 +54:44:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191684_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191684_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 191687_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191687_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:15:32.53 +49:04:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191690_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191690_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:17:49.61 +50:50:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191691_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191691_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191692_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191692_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 191693_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191693_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191696_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191696_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:48:52.44 +54:02:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191697_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191697_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:54:27.83 +57:13:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191699_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191699_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:20:28.68 +53:17:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191700_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191700_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:22.90 +57:23:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191701_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191701_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 191702_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191702_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:13:51.78 +53:25:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191706_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191706_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191708_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191708_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191709_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191709_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191710_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191710_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:54:30.33 +55:45:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191711_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191711_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (33.3") between the two second-epoch detections
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Considering the candidate 191712_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191712_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:21:47.08 +54:49:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191716_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191716_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 191717_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191717_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:48:12.06 +56:57:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191718_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191718_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:40.27 +55:59:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191719_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191719_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191721_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191721_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:28:09.84 +52:30:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191722_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191722_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:03.49 +50:30:46.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191724_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191724_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:09.72 +49:21:15.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191734_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191734_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:48.70 +49:01:18.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191736_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191736_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:58.26 +51:26:43.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191738_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191738_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:59.54 +49:04:10.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191740_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191740_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:45.36 +48:57:10.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191743_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191743_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:24.99 +51:05:40.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191752_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191752_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:34.67 +49:34:22.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191754_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191754_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:42.55 +49:49:59.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191755_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191755_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:30.86 +51:05:55.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191756_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191756_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:15.27 +48:33:11.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191763_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191763_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:09.33 +49:58:03.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191767_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191767_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:31:52.54 +48:39:21.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191771_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191771_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:56.09 +49:20:54.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191772_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191772_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:26.90 +49:53:40.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191785_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191785_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:51.03 +49:50:45.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191790_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191790_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:28.16 +50:24:36.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191792_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191792_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:15.35 +49:44:53.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191796_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191796_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:11.51 +50:39:12.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191808_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191808_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:39.70 +50:41:41.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191815_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191815_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 191819_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191819_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:31.33 +49:33:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191820_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191820_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:37.58 +50:29:03.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191822_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191822_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:43.75 +48:49:43.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191845_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191845_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:46.51 +50:16:12.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191847_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191847_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:55.81 +50:17:22.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191850_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191850_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:21.50 +50:18:27.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191851_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191851_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:09.90 +49:02:17.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 191860_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191860_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:41.94 +51:41:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191865_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191865_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 191869_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191869_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 191870_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191870_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:56.14 +49:37:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191874_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191874_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:08.07 +51:42:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191876_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191876_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 191880_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191880_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:54.26 +50:30:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191882_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191882_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 191886_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191886_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:24.64 +49:35:29.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 191887_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191887_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:17.66 +51:32:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191889_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191889_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:56.93 +49:24:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191899_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191899_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191900_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191900_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:34:23.54 +49:19:33.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 191902_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191902_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:48:57.03 +51:47:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191907_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191907_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 191914_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191914_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 191915_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191915_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:40.12 +49:34:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191917_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191917_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:27:48.36 +48:44:52.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 191921_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191921_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:20.30 +49:36:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191923_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191923_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:14.46 +50:00:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191926_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191926_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:31.89 +50:22:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191929_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191929_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191935_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191935_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:00.31 +50:06:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191939_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191939_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:50.82 +50:22:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191940_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191940_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:41.46 +49:37:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191950_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 191950_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 191957_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191957_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:29:36.70 +48:43:49.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 191962_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191962_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:46.00 +49:22:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191973_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191973_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:23.58 +50:04:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191978_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191978_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:12.47 +50:26:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191979_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191979_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:33:15.77 +49:05:58.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 191980_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191980_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:58.22 +49:52:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191982_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191982_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:15.03 +50:07:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191990_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 191990_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192001_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192001_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:11.78 +49:53:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192002_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192002_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192005_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192005_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:28.31 +49:30:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192009_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192009_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192010_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192010_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:08.05 +49:26:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192012_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192012_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:34:29.46 +49:19:02.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192015_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192015_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:46.83 +50:46:19.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192020_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192020_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:56.80 +48:55:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192022_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192022_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:13.70 +50:40:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192027_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192027_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:50.19 +49:42:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192040_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192040_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:26.24 +50:06:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192045_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192045_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:51.28 +49:49:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192047_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192047_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192048_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192048_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:31:30.18 +49:04:17.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192049_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192049_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:14.11 +49:12:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192050_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192050_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:24.16 +50:56:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192052_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192052_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:47.77 +49:14:14.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192057_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192057_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:22.77 +49:20:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192058_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192058_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192064_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192064_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 192065_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192065_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:34:30.70 +49:44:37.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192066_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192066_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:31.34 +49:59:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192071_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192071_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:34.20 +50:17:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192072_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192072_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192073_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192073_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:19.16 +50:11:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192077_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192077_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:24.82 +50:55:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192078_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192078_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:59.30 +49:31:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192079_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192079_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:14.77 +49:18:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192083_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192083_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:10.71 +50:37:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192084_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192084_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:23.03 +49:46:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192099_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192099_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192107_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192107_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:42.85 +49:24:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192109_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192109_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:03.18 +49:14:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192110_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192110_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:49.10 +50:22:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192116_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192116_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192119_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192119_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:12.67 +49:28:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192124_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192124_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192145_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192145_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:20.43 +50:33:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192152_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192152_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:26.05 +49:32:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192155_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192155_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:48.76 +49:19:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192160_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192160_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:04.90 +50:22:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192161_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192161_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:02.10 +51:25:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192163_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192163_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:06.65 +50:14:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192167_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192167_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:27.00 +50:36:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192176_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192176_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:30:23.36 +48:54:32.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192182_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192182_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:29.22 +50:21:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192183_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192183_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:10.59 +50:33:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192185_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192185_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:10.03 +49:39:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192188_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192188_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:38.78 +49:51:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192196_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192196_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:31.89 +50:07:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192199_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192199_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192201_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192201_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:16.46 +49:55:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192202_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192202_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:32:51.81 +49:19:39.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192206_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192206_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:48:02.28 +50:47:44.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192207_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192207_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:18.50 +49:41:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192221_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192221_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:28.65 +50:46:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192223_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192223_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192225_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192225_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:13.16 +50:03:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192228_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192228_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:53.63 +50:43:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192232_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192232_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:46.12 +48:49:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192234_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192234_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:27:08.00 +48:44:41.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192235_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192235_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:32:49.67 +49:11:26.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192236_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192236_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:37.54 +49:38:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192241_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192241_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:32.48 +50:35:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192243_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192243_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:03.53 +48:45:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192245_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192245_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:27.44 +50:43:41.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192254_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192254_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:50.20 +49:59:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192263_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192263_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:09.41 +49:16:34.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192267_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192267_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:11.64 +50:07:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192276_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192276_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:20.39 +51:46:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192281_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192281_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192289_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192289_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:57.94 +50:23:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192294_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192294_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192296_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192296_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:35.23 +48:51:39.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192302_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192302_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:24.58 +49:11:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192312_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192312_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192321_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192321_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192322_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192322_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:50.71 +49:48:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192323_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192323_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:48.50 +50:46:25.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192325_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192325_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:23.81 +51:49:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192327_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192327_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:52.35 +49:24:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192328_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192328_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:34:00.99 +49:25:53.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192329_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192329_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:37.52 +50:13:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192333_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192333_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:48:26.64 +51:34:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192342_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192342_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:17.22 +57:38:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192348_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192348_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192353_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192353_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:22.58 +49:43:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192361_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192361_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:48.00 +50:36:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192370_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192370_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:43.74 +49:56:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192372_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192372_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:26.46 +49:31:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192375_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192375_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 192383_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192383_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:04.02 +50:08:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192385_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192385_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:34:40.10 +48:54:44.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192387_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192387_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 192390_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192390_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:33:37.42 +49:04:29.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192398_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192398_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192399_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192399_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:58.54 +50:41:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192402_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192402_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 192409_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192409_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192411_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192411_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192419_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192419_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:41.14 +49:06:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192421_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192421_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:52.99 +49:12:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192424_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192424_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:19.62 +49:49:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192425_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192425_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:46.39 +50:08:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192429_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192429_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:17.93 +49:27:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192430_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192430_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192438_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192438_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:39.24 +50:00:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192439_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192439_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192440_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192440_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:34:32.57 +48:57:00.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192442_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192442_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 192449_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192449_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:31:24.71 +49:05:00.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192450_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192450_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192453_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192453_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:03.61 +49:44:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192458_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192458_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192462_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192462_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:42.33 +50:19:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192464_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192464_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:09.21 +50:35:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192467_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192467_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192471_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192471_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:27:26.41 +49:36:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192475_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192475_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192477_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192477_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:22.89 +49:09:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192478_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192478_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:24.05 +48:47:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192481_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192481_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:14.57 +49:42:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192484_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192484_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:16.03 +51:51:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192486_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192486_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:14.10 +49:05:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192489_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192489_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:21.52 +50:46:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192492_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192492_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192493_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192493_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:52.63 +49:17:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192500_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192500_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:34:57.76 +49:53:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192503_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192503_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:20.64 +49:30:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192505_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192505_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192510_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192510_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:31.67 +50:10:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192513_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192513_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:38.48 +49:45:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192517_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192517_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192522_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192522_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:21.71 +49:38:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192528_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192528_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:37.90 +49:11:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192532_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192532_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192534_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192534_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192547_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192547_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192548_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192548_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:28.52 +49:47:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192549_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192549_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192550_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192550_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:24.64 +50:04:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192555_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192555_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192557_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192557_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192566_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192566_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:03.64 +50:06:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192567_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192567_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192568_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192568_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192581_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192581_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:44.22 +49:33:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192589_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192589_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:36.84 +49:46:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192591_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192591_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:24.72 +50:53:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192604_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192604_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192605_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192605_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192608_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192608_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192613_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192613_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:11.48 +49:27:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192620_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192620_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192622_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192622_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192632_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192632_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:32.42 +49:52:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192633_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192633_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192641_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192641_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192644_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192644_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:55.33 +50:23:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192646_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192646_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192657_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192657_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192667_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192667_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:48.76 +49:28:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192670_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192670_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192676_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192676_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192677_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192677_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192678_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192678_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:35.83 +50:26:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192685_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192685_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:22.84 +50:18:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192689_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192689_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192691_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192691_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:53.97 +49:24:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192692_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192692_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:43.57 +49:08:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192693_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192693_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:24.30 +50:02:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192697_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192697_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:03.26 +49:34:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192701_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192701_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192703_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192703_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192706_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192706_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:18.06 +49:53:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192707_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192707_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192708_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192708_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192711_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192711_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:48:33.22 +51:46:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192713_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192713_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:07.37 +50:08:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192716_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192716_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:46.39 +49:50:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192719_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192719_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:44.49 +49:19:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192720_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192720_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192721_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192721_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:34.07 +50:28:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192723_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192723_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:17.40 +49:10:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192726_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192726_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:09.19 +49:18:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192731_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192731_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192732_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192732_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:24.74 +49:51:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192733_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192733_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192741_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192741_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:26.81 +49:13:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192744_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192744_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:35.69 +49:44:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192749_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192749_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:29.34 +49:24:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192753_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192753_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192757_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192757_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 192759_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192759_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192762_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192762_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192763_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192763_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:24.24 +50:17:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192764_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192764_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192771_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192771_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:16.67 +50:16:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192773_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192773_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:32.65 +50:11:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192775_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192775_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192778_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192778_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:49.92 +49:31:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192793_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192793_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:29.95 +50:25:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192795_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192795_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:33.35 +50:27:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192800_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192800_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:05.49 +50:27:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192801_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192801_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:16.67 +50:22:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192816_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192816_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192817_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192817_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:06.27 +49:35:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192819_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192819_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:48:26.25 +54:48:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192823_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192823_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192826_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192826_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192827_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192827_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:38.68 +49:20:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.63, MAG_FAINT_SEARCH_LIMIT=10.61)GAIADR2_OUTPUT=# 4.430 414636937329251712 010.90981523987 +49.34880431745 10.6061 10.3836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 192828_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192828_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:26.99 +49:15:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192829_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192829_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:22.96 +50:03:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192840_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192840_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:45.86 +49:47:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192841_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192841_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192846_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192846_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 192847_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192847_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:02.47 +49:43:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192854_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192854_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192858_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192858_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:13.75 +50:57:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192859_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192859_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:25.60 +49:05:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192861_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192861_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192864_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192864_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:02.99 +50:08:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192867_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192867_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192868_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192868_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:52:24.01 +55:37:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192869_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192869_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:35.15 +48:58:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192872_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192872_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:09.21 +49:43:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192877_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192877_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 192879_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192879_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192880_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192880_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:01.52 +49:39:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192884_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192884_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:56.17 +49:44:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192893_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192893_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:55.98 +49:36:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192895_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192895_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:39.81 +49:47:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192898_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192898_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:31.79 +51:43:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192900_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192900_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:48.10 +50:18:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192904_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192904_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 192908_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192908_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192910_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192910_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:57.61 +49:19:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192911_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192911_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (44.3") between the two second-epoch detections
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Considering the candidate 192912_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192912_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192918_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192918_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:53.98 +50:01:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192920_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192920_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192926_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192926_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:15:53.64 +57:50:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192928_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192928_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192929_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192929_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192930_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192930_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192937_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192937_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:57.75 +49:39:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192942_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192942_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192945_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192945_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 192946_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192946_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:33.51 +51:47:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192949_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192949_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192951_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192951_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:50.16 +49:44:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192953_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192953_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:53.77 +50:11:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192954_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192954_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192957_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192957_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192959_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192959_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:22.11 +50:19:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192969_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192969_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 192975_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 192975_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 192987_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 192987_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193004_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193004_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193005_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193005_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:54.01 +50:41:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193007_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193007_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:02.83 +50:09:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193009_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193009_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:11.09 +50:02:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193010_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193010_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193012_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193012_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193030_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193030_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193032_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193032_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193034_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193034_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193035_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193035_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:33.65 +49:30:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193036_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193036_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:13:08.88 +53:45:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193060_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193060_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193062_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193062_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:53.75 +49:30:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193065_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193065_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193070_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193070_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193077_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193077_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:06.14 +49:24:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193079_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193079_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:49.87 +49:52:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193081_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193081_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193086_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193086_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193091_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193091_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193094_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193094_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:29.10 +49:55:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193105_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193105_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:26.25 +50:10:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193115_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193115_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:16.19 +50:16:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193117_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193117_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:10.90 +49:37:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193121_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193121_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:21.97 +49:35:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193123_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193123_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193125_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193125_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:06.37 +49:52:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193127_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193127_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:18.71 +49:52:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193130_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193130_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193133_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193133_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193137_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193137_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:25.50 +51:45:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193139_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193139_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:03.35 +50:26:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193140_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193140_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193144_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193144_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 193145_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193145_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:28.36 +49:35:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193146_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193146_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:02.58 +50:19:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193151_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193151_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193164_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193164_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193165_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193165_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:35.26 +50:17:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193168_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193168_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193169_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193169_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193170_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193170_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:40.27 +50:34:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193175_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193175_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:25.26 +49:54:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193181_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193181_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193182_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193182_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193183_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193183_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:10.25 +49:19:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193189_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193189_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193190_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193190_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193193_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193193_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:33.80 +50:23:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193195_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193195_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:30.41 +51:32:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193196_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193196_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193199_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193199_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193200_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193200_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193202_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193202_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:47.97 +50:28:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193205_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193205_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193206_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193206_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 193218_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193218_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 193220_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193220_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193221_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193221_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:07.76 +50:48:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193225_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193225_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193227_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193227_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193231_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193231_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:24.41 +50:08:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193244_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193244_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:13.93 +50:30:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193246_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193246_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193249_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193249_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:38.51 +49:29:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193250_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193250_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:26.79 +56:45:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193253_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193253_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193254_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193254_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:51.65 +49:38:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193259_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193259_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193262_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193262_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:06.34 +50:31:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193263_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193263_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193264_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193264_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193268_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193268_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193273_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193273_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193280_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193280_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193284_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193284_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:35.10 +49:37:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193288_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193288_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193291_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193291_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193293_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193293_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193300_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193300_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193302_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193302_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193307_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193307_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:04.08 +50:20:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193311_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193311_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193313_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193313_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:42.86 +49:23:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193316_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193316_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193318_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193318_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193326_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193326_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193328_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193328_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:14.51 +49:48:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193330_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193330_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193332_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193332_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:26.28 +49:27:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193335_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193335_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193338_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193338_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193339_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193339_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193345_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193345_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193346_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193346_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:35:25.61 +49:55:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193353_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193353_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:54:36.50 +57:28:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193354_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193354_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:46.22 +56:07:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193369_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193369_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:07.30 +50:01:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193370_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193370_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:12:28.23 +57:05:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193379_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193379_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:10.66 +49:04:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193390_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193390_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:42:07.26 +57:15:39.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193393_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193393_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193395_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193395_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193396_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193396_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193398_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193398_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193401_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193401_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193403_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193403_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:25:37.29 +53:21:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193407_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193407_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:12.65 +49:52:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193408_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193408_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193410_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193410_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193412_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193412_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:39.63 +50:04:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193415_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193415_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:23:03.76 +55:45:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193417_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193417_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193426_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193426_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193427_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193427_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:59:23.83 +50:31:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193429_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193429_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193430_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193430_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193434_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193434_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 193445_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193445_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193446_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193446_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193450_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193450_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193451_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193451_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193470_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193470_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193479_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193479_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:38.66 +49:24:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193483_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193483_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193487_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193487_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193489_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193489_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193491_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193491_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193493_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193493_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193500_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193500_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193501_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193501_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193504_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193504_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:56:37.15 +57:16:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193507_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193507_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:07:30.70 +54:51:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193509_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193509_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193510_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193510_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193512_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193512_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193514_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193514_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:52:59.75 +57:15:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193520_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193520_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193522_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193522_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193524_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193524_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193525_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193525_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193531_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193531_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193532_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193532_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193534_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193534_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 193536_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193536_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:44.56 +56:31:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193537_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193537_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:34.66 +49:09:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193540_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193540_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193553_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193553_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:05.14 +57:09:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193561_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193561_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193562_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193562_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193564_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193564_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193568_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193568_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193569_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193569_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193571_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193571_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193575_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193575_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:21:47.71 +55:43:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193578_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193578_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193581_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193581_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193588_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193588_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193593_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193593_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:00.82 +49:52:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193594_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193594_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:21.08 +49:51:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193595_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193595_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193596_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193596_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193607_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193607_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:07:20.74 +54:49:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193611_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193611_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193613_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193613_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193614_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193614_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 193615_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193615_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:21:11.91 +50:00:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 3.096 1991161548689209984 350.29831220230 +50.00333248370 9.7912 8.5016 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 193618_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193618_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:36.25 +50:05:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193620_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193620_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:35.96 +49:07:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193628_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193628_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:52:07.61 +55:48:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193637_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193637_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193639_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193639_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193643_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193643_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193646_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193646_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193647_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193647_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193648_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193648_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193655_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193655_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193656_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193656_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193657_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193657_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:42.13 +49:07:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193662_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193662_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:42.83 +58:02:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193663_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193663_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:53:28.24 +57:37:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193664_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193664_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193672_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193672_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193673_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193673_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 193675_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193675_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193677_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193677_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193681_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193681_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193690_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193690_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193693_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193693_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:34.81 +49:11:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193700_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193700_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:30.89 +50:35:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193705_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193705_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193706_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193706_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193708_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193708_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193712_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193712_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:23.82 +48:52:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193713_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193713_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193714_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193714_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193716_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193716_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193717_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193717_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 193718_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193718_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 193720_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193720_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193722_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193722_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193723_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193723_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193726_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193726_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193728_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193728_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193731_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193731_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193734_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193734_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193736_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193736_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193742_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193742_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193743_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193743_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:03.72 +54:11:28.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193746_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193746_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193775_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193775_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193779_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193779_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193783_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193783_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193785_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193785_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193786_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193786_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193787_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193787_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193788_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193788_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:38.80 +48:57:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193794_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193794_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 193796_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193796_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193797_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193797_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193799_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193799_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 193803_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193803_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:07.82 +49:23:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193807_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193807_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:48:14.07 +52:57:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193809_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193809_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:39.81 +49:35:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193810_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193810_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193825_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193825_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:39.77 +50:17:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193829_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193829_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:56.05 +49:21:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193836_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193836_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193842_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193842_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193843_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193843_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193847_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193847_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193848_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193848_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193852_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193852_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 193853_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193853_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:06.77 +57:19:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193855_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193855_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193859_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193859_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:12:10.63 +52:47:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193862_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193862_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:36.81 +49:32:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193870_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193870_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193872_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193872_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193873_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193873_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193878_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193878_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:00.90 +49:24:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193879_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193879_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193882_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193882_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193889_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193889_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193891_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193891_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 193893_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193893_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193897_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193897_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193899_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193899_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193901_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193901_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:47:21.46 +50:39:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193902_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193902_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:49:03.08 +57:04:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193903_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193903_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:06.92 +57:18:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193907_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193907_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193910_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193910_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193911_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193911_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193912_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193912_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193913_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193913_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193929_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193929_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193931_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193931_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 193932_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193932_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193935_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193935_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193936_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193936_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193940_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193940_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:52.22 +50:28:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193943_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193943_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193944_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193944_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:51.77 +50:40:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193946_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193946_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193956_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193956_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193965_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193965_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193966_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193966_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193970_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193970_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193976_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193976_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 193978_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193978_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 193981_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193981_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193983_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193983_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193993_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193993_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 193994_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193994_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193995_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193995_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193996_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 193996_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 193999_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 193999_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:32.45 +49:31:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194002_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194002_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194003_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194003_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194004_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194004_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194005_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194005_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:10:56.06 +56:50:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194011_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194011_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194017_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194017_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:14:25.61 +55:24:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194020_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194020_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:17:48.32 +55:05:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194021_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194021_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194022_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194022_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 194025_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194025_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194026_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194026_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:57:07.18 +55:40:46.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194030_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194030_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:19:31.83 +55:36:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194033_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194033_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194038_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194038_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194042_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194042_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:06:18.02 +57:18:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194043_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194043_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:28.17 +50:17:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194044_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194044_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 194053_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194053_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194060_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194060_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194064_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194064_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194070_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194070_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194079_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194079_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194080_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194080_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:11.70 +49:42:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194082_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194082_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194083_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194083_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194086_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194086_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:03.62 +50:27:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194088_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194088_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:05:42.62 +58:17:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194089_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194089_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194095_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194095_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194099_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194099_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:38.05 +50:37:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194106_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194106_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194109_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194109_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194114_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194114_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194118_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194118_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194122_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194122_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194124_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194124_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194128_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194128_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194130_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194130_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194131_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194131_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194133_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194133_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194138_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194138_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194142_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194142_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:27.43 +50:35:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194144_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194144_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194149_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194149_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194154_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194154_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194163_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194163_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194179_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194179_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194189_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194189_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194194_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194194_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194195_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194195_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194202_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194202_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194206_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194206_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194209_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194209_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194213_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194213_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194218_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194218_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194221_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194221_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194224_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194224_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194230_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194230_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194232_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194232_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:46.59 +56:08:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194242_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194242_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194243_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194243_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194245_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194245_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194246_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194246_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194247_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194247_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194254_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194254_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194255_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194255_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194258_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194258_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194267_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194267_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194268_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194268_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194280_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194280_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194282_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194282_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194285_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194285_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:54.29 +49:53:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194287_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194287_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194296_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194296_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:06.55 +49:35:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194302_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194302_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:58.55 +49:31:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194303_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194303_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194306_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194306_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194311_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194311_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194321_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194321_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194332_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194332_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194333_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194333_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:06:33.10 +56:43:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194345_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194345_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194347_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194347_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194349_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194349_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194350_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194350_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194358_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194358_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:10:37.18 +57:00:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194359_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194359_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194360_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194360_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:37:11.01 +58:00:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194363_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194363_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:21:04.18 +57:36:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194367_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194367_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:18:53.47 +56:27:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194370_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194370_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194380_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194380_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194381_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194381_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194384_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194384_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194387_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194387_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194388_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194388_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194396_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194396_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194397_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194397_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194403_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194403_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194407_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194407_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194408_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194408_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194412_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194412_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194414_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194414_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194418_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194418_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194425_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194425_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194426_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194426_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194427_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194427_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194430_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194430_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194431_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194431_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:13:37.72 +56:24:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194433_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194433_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194440_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194440_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194441_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194441_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194448_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194448_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194456_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194456_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194464_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194464_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:24.55 +49:36:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 3.735 414657411435722624 011.60124459267 +49.61370166549 11.6442 11.1356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 194467_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194467_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194468_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194468_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:22.67 +49:00:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194469_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194469_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194471_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194471_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:17:27.07 +56:29:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194472_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194472_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194477_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194477_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194482_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194482_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194484_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194484_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194485_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194485_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194494_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194494_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:04.13 +50:21:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194496_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194496_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194504_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194504_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194506_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194506_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194508_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194508_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194512_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194512_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194513_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194513_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194517_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194517_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194531_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194531_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:45:29.24 +49:26:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194533_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194533_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194537_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194537_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194538_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194538_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194539_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194539_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194544_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194544_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194556_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194556_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194560_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194560_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194565_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194565_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194567_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194567_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194574_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194574_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194584_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194584_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 194585_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194585_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194586_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194586_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194588_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194588_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194594_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194594_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194602_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194602_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194605_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194605_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194613_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194613_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194619_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194619_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194622_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194622_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194623_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194623_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194628_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194628_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194633_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194633_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194637_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194637_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194642_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194642_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:36.28 +48:54:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194644_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194644_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194651_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194651_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194656_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194656_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:17:56.56 +53:10:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194667_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194667_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:58.59 +50:13:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194669_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194669_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194677_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194677_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194678_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194678_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194681_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194681_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194683_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194683_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194696_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194696_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194709_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194709_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:10:43.09 +57:31:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194712_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194712_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 194713_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194713_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194714_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194714_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:58.57 +49:29:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194719_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194719_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:55.62 +49:59:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194720_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194720_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:31:43.28 +56:11:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194725_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194725_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194732_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194732_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194733_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194733_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194734_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194734_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:28:20.94 +54:48:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194736_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194736_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194738_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194738_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194741_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194741_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194744_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194744_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194746_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194746_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194747_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194747_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 194748_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194748_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194749_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194749_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:25.98 +49:14:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194751_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194751_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (69.3") between the two second-epoch detections
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Considering the candidate 194759_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194759_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194766_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194766_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194768_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194768_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:28:14.03 +57:49:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194771_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194771_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194774_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194774_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194775_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194775_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:56.31 +48:45:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194782_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194782_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194783_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194783_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194790_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194790_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194792_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194792_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194794_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194794_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:09:24.52 +55:39:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194804_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194804_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194805_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194805_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194809_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194809_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194813_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194813_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:53:28.02 +57:04:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194817_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194817_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194823_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194823_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194824_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194824_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194831_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194831_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194834_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194834_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194838_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194838_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194839_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194839_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194845_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194845_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194847_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194847_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194859_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194859_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194874_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194874_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194875_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194875_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194881_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194881_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194884_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194884_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:27:11.67 +53:53:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194885_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194885_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:59:07.03 +53:34:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194892_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194892_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194903_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194903_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:15:35.02 +57:14:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194904_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194904_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 194905_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194905_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194908_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194908_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194910_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194910_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:38:16.46 +48:52:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194912_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194912_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:20.74 +49:13:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194924_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194924_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194934_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194934_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194937_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194937_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194938_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194938_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194946_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194946_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194952_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194952_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194953_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194953_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:09:03.56 +56:22:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194954_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194954_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 194956_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194956_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194960_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194960_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:00:37.78 +56:39:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194963_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194963_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194967_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194967_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194969_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194969_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194971_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194971_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:43:28.54 +50:38:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194974_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194974_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194976_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194976_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:46:31.17 +49:49:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194988_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194988_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 194993_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 194993_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 194996_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 194996_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195022_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195022_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195026_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195026_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:49:47.18 +56:38:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195033_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195033_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:51:14.63 +56:34:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195035_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195035_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195046_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195046_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195047_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195047_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 195049_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195049_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195053_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195053_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195056_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195056_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195058_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195058_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195065_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195065_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195071_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195071_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195094_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195094_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195095_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195095_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:41:21.65 +49:03:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195096_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195096_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195101_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195101_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 195102_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195102_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:17:01.15 +56:23:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195117_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195117_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:40:10.96 +49:26:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195121_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195121_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195122_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195122_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:56:18.03 +56:10:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195156_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195156_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:43:15.37 +51:56:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195175_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195175_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 195180_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195180_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195182_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195182_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195186_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195186_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195188_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195188_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195189_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195189_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195194_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195194_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195195_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195195_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195199_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195199_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 195242_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195242_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195244_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195244_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195245_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195245_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 195251_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195251_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 195255_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195255_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195261_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195261_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 195269_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195269_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195272_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195272_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:39.72 +48:54:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195277_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195277_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195289_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195289_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195291_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195291_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195312_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195312_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 195313_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195313_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195322_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195322_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195337_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195337_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195340_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195340_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195343_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195343_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 195345_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195345_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:11.17 +49:16:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195364_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195364_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195366_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195366_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195381_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195381_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195398_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195398_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195401_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195401_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195409_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195409_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195415_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195415_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195419_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195419_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195423_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195423_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195431_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195431_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 195433_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195433_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:39:13.87 +50:01:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195439_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195439_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:44.96 +50:21:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195450_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195450_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195495_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195495_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195500_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195500_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:44:32.05 +49:28:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195512_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195512_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195560_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195560_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195561_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195561_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195562_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195562_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195578_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195578_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:08:36.78 +55:38:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195617_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195617_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195630_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195630_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195636_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 195636_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 195644_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195644_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
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Considering the candidate 195685_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 195685_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 35276_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 35276_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:58:25.13 +51:23:22.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 130627_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 130627_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 179362_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 179362_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:15:50.95 +57:32:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157807_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 157807_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 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 142400_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 142400_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 102002_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 102002_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 43197_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 43197_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
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Considering the candidate 75760_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 75760_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:26:05.94 +53:55:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143447_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 143447_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:51:53.36 +55:59:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105020_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 105020_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:09:20.61 +54:44:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35911_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 35911_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:09:36.68 +51:34:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134698_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 134698_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:09:24.53 +56:11:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164776_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 164776_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:07:38.31 +56:57:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.25, MAG_FAINT_SEARCH_LIMIT=11.23)GAIADR2_OUTPUT=# 4.151 2009155297006423552 346.91140387241 +56.95153985820 10.6221 9.1853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 178709_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 178709_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:42:10.14 +50:03:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178259_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
Preparing report for the candidate 178259_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121238_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 121238_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:36:01.35 +57:54:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100304_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 100304_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:20:22.38 +54:45:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139426_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 139426_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:11:31.39 +56:01:29.0 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37075_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 37075_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:41:31.07 +51:32:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105722_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 105722_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 00:04:40.79 +55:32:15.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140320_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123
The candidate 140320_fd_Cas-04-Q1b1x1_2026-07-09_23-46-13_20.00sec_-0.00C_LIGHTs_0123 did not pass the final checks
**** FOUND 23:44:31.76 +56:34:52.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 42s
make_report_in_HTML.sh TOTAL: 891s
Prepared the HTML report for the field Cas-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:35:09.93 +49:02:17.0
00:34:23.57 +49:19:33.0
00:27:48.38 +48:44:52.3
00:29:36.73 +48:43:49.9
00:46:53.36 +50:47:03.4
00:33:15.80 +49:05:57.8
00:44:46.84 +50:46:19.3
00:34:29.49 +49:19:02.2
00:31:30.22 +49:04:17.1
00:37:47.79 +49:14:14.2
00:34:30.75 +49:44:36.9
23:11:31.33 +56:01:29.3
00:44:04.93 +49:03:55.9
00:30:23.39 +48:54:32.5
00:32:51.85 +49:19:38.8
00:48:02.30 +50:47:44.6
00:27:08.02 +48:44:41.6
00:32:49.72 +49:11:25.7
00:35:09.45 +49:16:34.4
00:45:27.46 +50:43:41.0
00:39:35.16 +48:51:40.5
23:36:42.81 +52:12:23.4
23:10:51.78 +54:50:07.5
00:34:01.04 +49:25:53.0
00:47:48.52 +50:46:25.5
00:33:37.46 +49:04:29.0
00:34:40.16 +48:54:44.3
00:45:56.32 +51:07:56.6
23:31:09.43 +54:16:19.7
23:16:48.80 +55:26:59.8
00:31:24.77 +49:05:00.4
00:34:32.63 +48:57:00.3
00:34:57.81 +49:53:58.7
00:53:12.38 +54:48:07.2
00:55:31.18 +56:33:11.6
23:57:50.00 +56:34:46.4
00:48:55.16 +53:00:35.8
00:25:03.08 +55:19:43.6
23:17:32.89 +51:47:07.0
00:04:11.16 +57:55:53.2
23:31:45.01 +54:09:37.0
00:30:29.22 +55:18:05.8
23:28:31.85 +53:36:18.8
00:42:52.90 +52:06:34.0
00:29:53.36 +50:13:53.1
00:43:19.98 +58:08:06.2
23:20:45.39 +53:43:33.9
00:31:10.05 +55:39:13.7
00:46:48.49 +58:10:11.1
00:53:07.27 +54:59:06.0
00:42:59.78 +51:05:48.6
00:29:48.44 +49:15:04.0
00:57:24.04 +57:00:13.7
00:32:01.16 +49:19:09.0
00:46:23.97 +49:40:43.6
00:39:11.67 +49:08:18.6
00:30:54.04 +49:16:44.7
00:43:48.42 +51:02:28.2
00:27:20.86 +48:44:02.2
00:45:30.28 +49:28:32.1
00:39:40.72 +49:07:27.9
00:46:31.50 +51:13:43.9
00:42:30.77 +50:54:50.5
00:39:56.30 +49:02:10.3
00:46:11.97 +50:44:47.5
00:46:04.86 +49:37:41.0
00:34:22.76 +49:57:18.7
00:34:03.66 +49:02:32.9
00:29:53.01 +50:05:46.7
00:31:51.19 +49:28:31.3
00:33:18.41 +49:37:35.2
00:34:02.57 +49:31:15.8
00:29:36.60 +48:56:00.8
00:34:08.69 +48:55:40.6
00:34:56.95 +48:53:46.8
00:43:58.21 +49:10:33.6
00:33:26.77 +49:19:04.2
00:30:37.49 +49:15:38.7
00:31:59.22 +49:09:55.8
00:33:05.91 +49:26:24.6
00:39:34.85 +48:54:30.4
00:30:09.72 +49:12:21.9
00:34:35.21 +49:51:37.2
00:47:47.57 +50:59:21.3
00:44:27.71 +50:58:49.6
00:30:43.92 +49:15:29.0
00:33:00.64 +49:33:16.6
00:42:56.93 +50:54:49.2
00:42:00.91 +50:58:01.7
00:34:52.01 +49:01:28.4
00:56:52.48 +57:23:42.3
00:35:17.56 +49:14:23.8
00:39:23.37 +48:58:48.7
00:40:58.27 +48:54:05.6
00:34:16.96 +49:38:26.3
00:39:42.16 +49:10:15.2
00:32:20.07 +49:32:47.4
00:34:04.42 +49:01:31.6
00:47:24.18 +50:34:15.5
00:34:36.11 +49:29:11.0
00:34:35.94 +49:33:31.0
00:26:50.36 +49:10:19.8
00:47:01.14 +51:22:05.0
00:32:52.96 +48:59:29.8
00:27:32.28 +48:49:11.3
00:38:16.91 +49:08:28.6
00:39:11.60 +50:29:50.6
00:48:12.06 +50:51:51.2
00:43:16.28 +49:08:58.6
00:31:33.33 +49:18:21.9
00:34:49.24 +49:02:01.6
00:34:33.44 +49:23:40.3
00:42:29.35 +50:06:33.1
00:46:53.59 +49:51:36.0
00:48:47.12 +51:11:36.0
00:34:43.02 +49:42:52.9
00:29:55.57 +49:08:55.6
00:46:18.32 +50:52:22.2
00:45:52.74 +50:50:45.3
00:41:44.34 +49:24:11.3
00:43:57.38 +51:14:00.1
00:30:57.89 +49:16:02.0
00:39:33.86 +49:10:19.8
00:47:37.20 +50:24:26.3
00:44:43.93 +49:42:46.0
00:46:47.03 +51:14:07.0
00:46:38.70 +50:41:13.3
00:45:35.72 +50:31:49.7
00:47:41.69 +50:47:29.4
00:36:30.32 +49:32:05.3
00:38:19.01 +49:03:44.9
00:33:07.73 +49:00:57.2
00:42:49.44 +50:06:14.3
00:29:41.61 +48:41:39.6
00:37:06.77 +48:54:59.7
00:42:34.61 +50:13:17.7
00:39:17.09 +49:07:03.5
00:35:23.59 +49:04:22.7
00:35:46.59 +49:23:09.7
00:39:01.48 +49:30:16.9
00:48:11.86 +50:59:22.9
00:36:24.00 +49:29:18.0
00:38:30.74 +49:12:54.0
00:33:51.13 +49:19:04.6
00:35:46.91 +49:26:55.0
00:30:09.45 +49:34:50.7
00:39:37.63 +49:24:22.0
00:42:54.09 +50:11:16.8
00:36:35.64 +49:09:00.6
00:43:05.25 +51:03:48.0
00:47:50.76 +51:30:48.7
00:44:29.36 +50:13:55.6
00:34:40.93 +49:36:47.7
00:34:23.47 +49:51:01.4
00:40:24.89 +49:16:21.4
00:45:44.72 +49:39:24.3
00:33:46.17 +49:46:08.2
00:39:17.65 +49:05:13.0
23:38:10.97 +52:49:00.8
00:34:24.15 +49:22:46.1
00:35:22.91 +49:49:47.5
00:30:52.73 +49:19:20.6
00:47:14.56 +50:21:14.0
00:45:21.83 +50:47:05.3
00:38:25.76 +49:06:31.7
00:45:52.36 +50:24:02.4
00:29:26.24 +49:15:18.3
00:46:46.22 +49:46:26.9
00:41:06.82 +49:38:11.5
00:25:46.33 +57:59:01.6
00:40:46.97 +50:18:52.3
00:47:53.87 +51:24:28.5
00:39:00.38 +49:13:32.7
00:38:51.17 +49:35:21.5
00:44:05.27 +49:44:08.0
00:38:26.79 +48:56:46.1
00:42:11.50 +50:45:53.0
00:38:58.05 +50:19:33.2
00:48:01.29 +53:47:45.1
00:44:58.37 +50:03:21.4
23:23:16.71 +52:26:44.9
00:46:51.47 +50:27:44.6
00:37:19.86 +49:22:16.7
00:45:46.68 +50:38:15.2
00:35:36.16 +49:54:16.9
00:38:59.19 +49:06:42.7
00:45:42.35 +51:05:26.9
00:41:21.50 +51:05:37.9
00:36:47.78 +49:20:39.3
00:48:36.44 +51:29:37.3
00:43:53.05 +50:11:02.3
00:43:11.52 +49:49:44.5
00:44:42.74 +49:41:44.6
00:43:09.86 +50:58:24.1
00:44:05.44 +50:43:01.4
00:29:55.38 +49:08:27.7
00:38:16.02 +50:15:21.6
00:47:41.64 +50:48:50.0
00:41:47.49 +50:16:05.0
00:47:16.25 +50:51:07.5
00:34:40.97 +49:51:06.3
00:44:26.66 +49:49:48.2
00:54:51.88 +56:45:46.4
00:49:49.28 +51:59:45.6
00:33:35.04 +48:58:44.3
00:36:32.00 +49:04:15.8
00:38:25.34 +50:36:26.1
00:34:55.96 +49:03:58.2
00:39:45.58 +48:44:26.7
23:08:57.49 +53:23:18.7
00:46:17.92 +49:55:56.4
00:41:29.60 +49:57:06.5
00:43:45.45 +50:34:56.0
00:47:07.85 +50:10:53.4
00:44:59.23 +50:13:07.3
23:35:49.76 +51:16:44.8
00:48:23.17 +54:48:53.2
00:46:00.47 +49:48:02.8
00:38:33.21 +48:51:35.5
00:29:32.59 +48:52:54.5
00:43:06.12 +50:04:43.7
00:44:09.72 +50:56:04.3
00:41:42.76 +49:30:08.8
00:32:51.73 +50:26:51.0
00:40:05.03 +49:06:39.4
00:38:46.06 +50:08:08.9
00:43:31.49 +50:48:15.7
00:43:50.67 +49:59:41.7
00:48:19.07 +50:56:33.0
00:36:40.92 +49:23:46.2
00:02:36.41 +55:35:39.4
00:43:11.46 +50:19:29.1
00:46:14.54 +50:13:40.4
00:39:37.61 +49:41:10.3
00:36:02.81 +49:16:40.5
00:43:49.95 +50:02:21.8
00:56:43.95 +57:23:36.4
00:36:35.81 +49:27:25.3
00:36:46.61 +49:32:55.0
00:41:12.81 +49:20:24.3
00:37:52.79 +49:45:39.9
00:44:04.96 +50:24:35.5
23:25:05.02 +55:05:34.3
00:41:28.09 +50:30:28.5
00:42:59.23 +50:16:22.0
00:39:41.88 +50:10:46.9
00:33:40.12 +49:45:25.6
00:50:42.09 +57:57:35.7
00:35:45.67 +49:13:52.9
00:41:29.77 +50:40:23.7
23:08:22.62 +55:49:47.2
00:42:57.24 +50:03:47.4
00:36:14.23 +49:21:55.9
00:48:48.54 +51:15:20.3
00:31:10.03 +49:14:57.5
00:36:55.44 +48:50:41.1
00:43:50.81 +49:27:00.4
00:33:05.52 +49:31:10.2
00:42:38.36 +51:09:47.4
00:43:42.89 +49:43:38.4
00:33:00.47 +49:11:35.9
00:28:15.88 +48:43:18.0
00:37:15.82 +50:03:05.3
23:49:50.08 +53:26:58.0
00:42:28.55 +49:30:37.3
00:47:33.94 +51:22:13.1
00:16:11.31 +49:15:05.4
00:40:29.52 +50:01:01.3
00:41:38.91 +50:27:39.9
00:31:56.92 +49:18:09.7
00:44:22.71 +49:48:54.5
00:37:42.99 +49:34:53.4
00:44:34.34 +50:15:23.5
00:33:38.04 +48:56:21.0
00:46:54.69 +50:39:25.0
00:43:14.24 +49:38:10.6
00:34:06.99 +49:36:32.0
00:41:52.51 +49:45:52.2
00:35:41.72 +49:31:18.6
00:38:37.19 +48:53:14.6
00:42:06.28 +50:45:22.0
00:49:00.11 +51:55:18.7
00:35:10.25 +49:13:30.4
00:45:35.04 +50:06:54.9
00:41:50.04 +50:11:56.9
00:43:26.77 +50:14:20.5
23:16:02.64 +53:58:02.4
00:44:12.55 +50:33:09.4
00:40:26.52 +49:52:04.2
00:40:17.36 +49:38:27.2
00:46:08.11 +50:17:34.9
00:36:53.34 +49:27:42.2
00:47:01.70 +50:42:52.3
00:38:01.64 +49:00:50.7
00:49:38.43 +51:51:57.0
00:47:48.94 +51:15:14.7
00:41:59.49 +49:46:29.2
00:43:19.16 +49:55:12.4
00:34:00.17 +49:37:27.3
00:46:15.15 +49:37:46.0
00:44:08.70 +49:37:08.8
00:41:18.79 +50:23:11.4
00:46:30.01 +51:10:00.8
00:46:45.82 +50:14:20.7
00:39:13.54 +49:40:17.3
00:28:11.92 +49:22:01.3
00:38:16.15 +49:02:55.2
23:29:14.19 +53:24:27.1
00:47:56.81 +51:05:58.0
00:42:02.11 +50:39:27.8
00:47:00.30 +58:07:18.8
00:37:00.43 +48:58:17.9
00:35:14.12 +50:03:26.3
00:45:54.99 +50:24:54.3
00:41:00.79 +49:46:02.8
00:37:13.07 +50:18:04.1
00:40:07.31 +50:28:21.6
00:44:56.27 +50:15:32.7
00:39:18.87 +49:31:19.9
00:29:08.31 +49:02:49.1
00:37:51.50 +49:25:31.9
00:34:37.06 +49:02:32.4
00:31:47.72 +49:24:29.2
00:46:18.71 +50:55:13.5
00:41:45.39 +49:38:15.5
00:35:42.35 +49:48:55.2
00:42:08.09 +49:34:51.3
00:30:23.86 +49:14:52.6
00:47:38.64 +51:01:39.2
00:42:11.39 +49:32:38.0
00:47:34.39 +50:57:36.5
00:43:34.41 +49:42:59.4
23:42:21.26 +57:04:54.2
00:41:20.21 +49:42:43.6
00:46:38.80 +50:30:06.2
00:41:29.89 +50:21:53.2
00:46:43.15 +49:55:58.5
00:41:55.96 +50:06:51.5
00:44:16.75 +50:19:50.6
00:43:00.03 +50:33:03.3
00:34:57.86 +49:17:03.0
00:31:58.44 +49:07:28.5
00:33:05.59 +49:06:48.4
00:36:42.33 +49:06:19.3
00:44:43.10 +50:10:15.0
00:30:19.86 +48:50:51.9
00:35:56.60 +48:58:49.7
23:33:41.18 +49:58:08.9
00:35:03.83 +50:12:02.8
00:35:50.04 +48:59:20.0
00:46:26.92 +51:18:33.0
00:33:59.40 +50:02:29.6
23:32:20.38 +54:04:39.5
00:30:06.84 +49:24:56.5
00:42:43.93 +50:52:44.5
00:38:46.94 +49:15:20.7
00:46:10.02 +50:39:38.1
00:42:52.48 +50:10:11.2
00:39:45.11 +50:27:52.4
00:36:50.92 +49:58:17.1
00:40:09.34 +49:54:02.9
00:45:36.48 +50:15:29.1
00:33:35.61 +49:08:21.9
00:43:54.83 +49:43:20.1
00:45:25.13 +51:00:06.9
00:36:02.94 +49:22:20.1
00:34:11.17 +49:07:20.9
00:46:39.22 +51:36:36.2
00:29:47.99 +49:19:48.4
00:35:06.30 +49:53:43.8
00:40:28.12 +50:15:58.0
00:36:12.15 +49:57:42.5
23:33:31.05 +52:42:15.6
00:33:31.39 +50:04:38.4
00:41:50.21 +50:26:18.5
00:28:14.13 +48:45:48.1
00:40:03.09 +48:49:47.8
00:44:45.05 +49:44:26.1
00:37:58.58 +49:59:06.2
00:46:09.87 +51:24:24.0
00:42:09.50 +50:18:51.6
00:41:07.40 +50:43:02.2
00:35:22.89 +49:14:54.1
00:31:28.00 +49:10:51.3
00:38:26.44 +50:13:43.8
00:33:11.13 +49:10:15.8
00:43:40.88 +49:57:32.0
00:45:01.41 +50:21:07.3
00:36:24.46 +50:09:02.1
00:45:08.56 +50:23:58.5
23:38:36.59 +57:11:43.8
00:44:37.90 +50:16:26.2
00:34:04.89 +49:39:52.6
00:45:43.06 +51:24:41.2
00:42:00.00 +49:31:12.7
23:25:30.77 +57:09:53.7
00:34:44.60 +49:41:17.9
00:30:19.81 +48:56:58.7
23:24:32.34 +57:07:12.4
00:39:21.14 +50:28:23.6
00:45:50.71 +50:35:01.8
00:41:27.08 +50:23:44.8
00:40:29.75 +49:05:50.1
00:43:25.12 +50:19:24.6
00:41:25.86 +49:49:30.6
00:42:02.89 +49:45:10.8
00:33:40.47 +49:11:41.2
00:36:35.35 +49:51:39.6
00:48:02.49 +51:33:32.7
00:47:02.28 +50:32:18.5
00:38:35.35 +48:55:17.9
00:38:29.97 +50:26:20.4
00:28:30.56 +49:04:19.4
00:12:08.83 +50:38:18.1
00:29:50.13 +48:49:10.3
00:30:50.84 +49:58:09.9
00:45:56.19 +51:22:51.1
00:43:44.44 +51:06:54.1
00:44:39.41 +51:41:05.1
########### Completed Cas-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
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00:44:39.41 +51:41:05.1
00:48:55.16 +53:00:35.8
###################################################################################
00:35:09.93 +49:02:17.0 -- not an asteroid (will add it to exclusion list)
00:34:23.57 +49:19:33.0 -- not an asteroid (will add it to exclusion list)
00:27:48.38 +48:44:52.3 -- not an asteroid (will add it to exclusion list)
00:29:36.73 +48:43:49.9 -- not an asteroid (will add it to exclusion list)
00:46:53.36 +50:47:03.4 -- not an asteroid (will add it to exclusion list)
00:33:15.80 +49:05:57.8 -- not an asteroid (will add it to exclusion list)
00:44:46.84 +50:46:19.3 -- not an asteroid (will add it to exclusion list)
00:34:29.49 +49:19:02.2 -- not an asteroid (will add it to exclusion list)
00:31:30.22 +49:04:17.1 -- not an asteroid (will add it to exclusion list)
00:37:47.79 +49:14:14.2 -- not an asteroid (will add it to exclusion list)
00:34:30.75 +49:44:36.9 -- not an asteroid (will add it to exclusion list)
23:11:31.33 +56:01:29.3 -- not an asteroid (will add it to exclusion list)
00:44:04.93 +49:03:55.9 -- not an asteroid (will add it to exclusion list)
00:30:23.39 +48:54:32.5 -- not an asteroid (will add it to exclusion list)
00:32:51.85 +49:19:38.8 -- not an asteroid (will add it to exclusion list)
00:48:02.30 +50:47:44.6 -- not an asteroid (will add it to exclusion list)
00:27:08.02 +48:44:41.6 -- not an asteroid (will add it to exclusion list)
00:32:49.72 +49:11:25.7 -- not an asteroid (will add it to exclusion list)
00:35:09.45 +49:16:34.4 -- not an asteroid (will add it to exclusion list)
00:45:27.46 +50:43:41.0 -- not an asteroid (will add it to exclusion list)
00:39:35.16 +48:51:40.5 -- not an asteroid (will add it to exclusion list)
23:36:42.81 +52:12:23.4 -- not an asteroid (will add it to exclusion list)
23:10:51.78 +54:50:07.5 -- not an asteroid (will add it to exclusion list)
00:34:01.04 +49:25:53.0 -- not an asteroid (will add it to exclusion list)
00:47:48.52 +50:46:25.5 -- not an asteroid (will add it to exclusion list)
00:33:37.46 +49:04:29.0 -- not an asteroid (will add it to exclusion list)
00:34:40.16 +48:54:44.3 -- not an asteroid (will add it to exclusion list)
00:45:56.32 +51:07:56.6 -- not an asteroid (will add it to exclusion list)
23:31:09.43 +54:16:19.7 -- not an asteroid (will add it to exclusion list)
23:16:48.80 +55:26:59.8 -- not an asteroid (will add it to exclusion list)
00:31:24.77 +49:05:00.4 -- not an asteroid (will add it to exclusion list)
00:34:32.63 +48:57:00.3 -- not an asteroid (will add it to exclusion list)
00:34:57.81 +49:53:58.7 -- not an asteroid (will add it to exclusion list)
00:25:03.08 +55:19:43.6 -- not an asteroid (will add it to exclusion list)
23:17:32.89 +51:47:07.0 -- not an asteroid (will add it to exclusion list)
00:04:11.16 +57:55:53.2 -- not an asteroid (will add it to exclusion list)
23:31:45.01 +54:09:37.0 -- not an asteroid (will add it to exclusion list)
00:30:29.22 +55:18:05.8 -- not an asteroid (will add it to exclusion list)
23:28:31.85 +53:36:18.8 -- not an asteroid (will add it to exclusion list)
00:42:52.90 +52:06:34.0 -- not an asteroid (will add it to exclusion list)
00:29:53.36 +50:13:53.1 -- not an asteroid (will add it to exclusion list)
00:43:19.98 +58:08:06.2 -- not an asteroid (will add it to exclusion list)
23:20:45.39 +53:43:33.9 -- not an asteroid (will add it to exclusion list)
00:31:10.05 +55:39:13.7 -- not an asteroid (will add it to exclusion list)
00:46:48.49 +58:10:11.1 -- not an asteroid (will add it to exclusion list)
00:53:07.27 +54:59:06.0 -- not an asteroid (will add it to exclusion list)
00:42:59.78 +51:05:48.6 -- not an asteroid (will add it to exclusion list)
00:29:48.44 +49:15:04.0 -- not an asteroid (will add it to exclusion list)
00:57:24.04 +57:00:13.7 -- not an asteroid (will add it to exclusion list)
00:32:01.16 +49:19:09.0 -- not an asteroid (will add it to exclusion list)
00:46:23.97 +49:40:43.6 -- not an asteroid (will add it to exclusion list)
00:39:11.67 +49:08:18.6 -- not an asteroid (will add it to exclusion list)
00:30:54.04 +49:16:44.7 -- not an asteroid (will add it to exclusion list)
00:43:48.42 +51:02:28.2 -- not an asteroid (will add it to exclusion list)
00:27:20.86 +48:44:02.2 -- not an asteroid (will add it to exclusion list)
00:45:30.28 +49:28:32.1 -- not an asteroid (will add it to exclusion list)
00:39:40.72 +49:07:27.9 -- not an asteroid (will add it to exclusion list)
00:46:31.50 +51:13:43.9 -- not an asteroid (will add it to exclusion list)
00:42:30.77 +50:54:50.5 -- not an asteroid (will add it to exclusion list)
00:39:56.30 +49:02:10.3 -- not an asteroid (will add it to exclusion list)
00:46:11.97 +50:44:47.5 -- not an asteroid (will add it to exclusion list)
00:46:04.86 +49:37:41.0 -- not an asteroid (will add it to exclusion list)
00:34:22.76 +49:57:18.7 -- not an asteroid (will add it to exclusion list)
00:34:03.66 +49:02:32.9 -- not an asteroid (will add it to exclusion list)
00:29:53.01 +50:05:46.7 -- not an asteroid (will add it to exclusion list)
00:31:51.19 +49:28:31.3 -- not an asteroid (will add it to exclusion list)
00:33:18.41 +49:37:35.2 -- not an asteroid (will add it to exclusion list)
00:34:02.57 +49:31:15.8 -- not an asteroid (will add it to exclusion list)
00:29:36.60 +48:56:00.8 -- not an asteroid (will add it to exclusion list)
00:34:08.69 +48:55:40.6 -- not an asteroid (will add it to exclusion list)
00:34:56.95 +48:53:46.8 -- not an asteroid (will add it to exclusion list)
00:43:58.21 +49:10:33.6 -- not an asteroid (will add it to exclusion list)
00:33:26.77 +49:19:04.2 -- not an asteroid (will add it to exclusion list)
00:30:37.49 +49:15:38.7 -- not an asteroid (will add it to exclusion list)
00:31:59.22 +49:09:55.8 -- not an asteroid (will add it to exclusion list)
00:33:05.91 +49:26:24.6 -- not an asteroid (will add it to exclusion list)
00:39:34.85 +48:54:30.4 -- not an asteroid (will add it to exclusion list)
00:30:09.72 +49:12:21.9 -- not an asteroid (will add it to exclusion list)
00:34:35.21 +49:51:37.2 -- not an asteroid (will add it to exclusion list)
00:47:47.57 +50:59:21.3 -- not an asteroid (will add it to exclusion list)
00:44:27.71 +50:58:49.6 -- not an asteroid (will add it to exclusion list)
00:30:43.92 +49:15:29.0 -- not an asteroid (will add it to exclusion list)
00:33:00.64 +49:33:16.6 -- not an asteroid (will add it to exclusion list)
00:42:56.93 +50:54:49.2 -- not an asteroid (will add it to exclusion list)
00:42:00.91 +50:58:01.7 -- not an asteroid (will add it to exclusion list)
00:34:52.01 +49:01:28.4 -- not an asteroid (will add it to exclusion list)
00:56:52.48 +57:23:42.3 -- not an asteroid (will add it to exclusion list)
00:35:17.56 +49:14:23.8 -- not an asteroid (will add it to exclusion list)
00:39:23.37 +48:58:48.7 -- not an asteroid (will add it to exclusion list)
00:40:58.27 +48:54:05.6 -- not an asteroid (will add it to exclusion list)
00:34:16.96 +49:38:26.3 -- not an asteroid (will add it to exclusion list)
00:39:42.16 +49:10:15.2 -- not an asteroid (will add it to exclusion list)
00:32:20.07 +49:32:47.4 -- not an asteroid (will add it to exclusion list)
00:34:04.42 +49:01:31.6 -- not an asteroid (will add it to exclusion list)
00:47:24.18 +50:34:15.5 -- not an asteroid (will add it to exclusion list)
00:34:36.11 +49:29:11.0 -- not an asteroid (will add it to exclusion list)
00:34:35.94 +49:33:31.0 -- not an asteroid (will add it to exclusion list)
00:26:50.36 +49:10:19.8 -- not an asteroid (will add it to exclusion list)
00:47:01.14 +51:22:05.0 -- not an asteroid (will add it to exclusion list)
00:32:52.96 +48:59:29.8 -- not an asteroid (will add it to exclusion list)
00:27:32.28 +48:49:11.3 -- not an asteroid (will add it to exclusion list)
00:38:16.91 +49:08:28.6 -- not an asteroid (will add it to exclusion list)
00:39:11.60 +50:29:50.6 -- not an asteroid (will add it to exclusion list)
00:48:12.06 +50:51:51.2 -- not an asteroid (will add it to exclusion list)
00:43:16.28 +49:08:58.6 -- not an asteroid (will add it to exclusion list)
00:31:33.33 +49:18:21.9 -- not an asteroid (will add it to exclusion list)
00:34:49.24 +49:02:01.6 -- not an asteroid (will add it to exclusion list)
00:34:33.44 +49:23:40.3 -- not an asteroid (will add it to exclusion list)
00:42:29.35 +50:06:33.1 -- not an asteroid (will add it to exclusion list)
00:46:53.59 +49:51:36.0 -- not an asteroid (will add it to exclusion list)
00:48:47.12 +51:11:36.0 -- not an asteroid (will add it to exclusion list)
00:34:43.02 +49:42:52.9 -- not an asteroid (will add it to exclusion list)
00:29:55.57 +49:08:55.6 -- not an asteroid (will add it to exclusion list)
00:46:18.32 +50:52:22.2 -- not an asteroid (will add it to exclusion list)
00:45:52.74 +50:50:45.3 -- not an asteroid (will add it to exclusion list)
00:41:44.34 +49:24:11.3 -- not an asteroid (will add it to exclusion list)
00:43:57.38 +51:14:00.1 -- not an asteroid (will add it to exclusion list)
00:30:57.89 +49:16:02.0 -- not an asteroid (will add it to exclusion list)
00:39:33.86 +49:10:19.8 -- not an asteroid (will add it to exclusion list)
00:47:37.20 +50:24:26.3 -- not an asteroid (will add it to exclusion list)
00:44:43.93 +49:42:46.0 -- not an asteroid (will add it to exclusion list)
00:46:47.03 +51:14:07.0 -- not an asteroid (will add it to exclusion list)
00:46:38.70 +50:41:13.3 -- not an asteroid (will add it to exclusion list)
00:45:35.72 +50:31:49.7 -- not an asteroid (will add it to exclusion list)
00:47:41.69 +50:47:29.4 -- not an asteroid (will add it to exclusion list)
00:36:30.32 +49:32:05.3 -- not an asteroid (will add it to exclusion list)
00:38:19.01 +49:03:44.9 -- not an asteroid (will add it to exclusion list)
00:33:07.73 +49:00:57.2 -- not an asteroid (will add it to exclusion list)
00:42:49.44 +50:06:14.3 -- not an asteroid (will add it to exclusion list)
00:29:41.61 +48:41:39.6 -- not an asteroid (will add it to exclusion list)
00:37:06.77 +48:54:59.7 -- not an asteroid (will add it to exclusion list)
00:42:34.61 +50:13:17.7 -- not an asteroid (will add it to exclusion list)
00:39:17.09 +49:07:03.5 -- not an asteroid (will add it to exclusion list)
00:35:23.59 +49:04:22.7 -- not an asteroid (will add it to exclusion list)
00:35:46.59 +49:23:09.7 -- not an asteroid (will add it to exclusion list)
00:39:01.48 +49:30:16.9 -- not an asteroid (will add it to exclusion list)
00:48:11.86 +50:59:22.9 -- not an asteroid (will add it to exclusion list)
00:36:24.00 +49:29:18.0 -- not an asteroid (will add it to exclusion list)
00:38:30.74 +49:12:54.0 -- not an asteroid (will add it to exclusion list)
00:33:51.13 +49:19:04.6 -- not an asteroid (will add it to exclusion list)
00:35:46.91 +49:26:55.0 -- not an asteroid (will add it to exclusion list)
00:30:09.45 +49:34:50.7 -- not an asteroid (will add it to exclusion list)
00:39:37.63 +49:24:22.0 -- not an asteroid (will add it to exclusion list)
00:42:54.09 +50:11:16.8 -- not an asteroid (will add it to exclusion list)
00:36:35.64 +49:09:00.6 -- not an asteroid (will add it to exclusion list)
00:43:05.25 +51:03:48.0 -- not an asteroid (will add it to exclusion list)
00:47:50.76 +51:30:48.7 -- not an asteroid (will add it to exclusion list)
00:44:29.36 +50:13:55.6 -- not an asteroid (will add it to exclusion list)
00:34:40.93 +49:36:47.7 -- not an asteroid (will add it to exclusion list)
00:34:23.47 +49:51:01.4 -- not an asteroid (will add it to exclusion list)
00:40:24.89 +49:16:21.4 -- not an asteroid (will add it to exclusion list)
00:45:44.72 +49:39:24.3 -- not an asteroid (will add it to exclusion list)
00:33:46.17 +49:46:08.2 -- not an asteroid (will add it to exclusion list)
00:39:17.65 +49:05:13.0 -- not an asteroid (will add it to exclusion list)
23:38:10.97 +52:49:00.8 -- not an asteroid (will add it to exclusion list)
00:34:24.15 +49:22:46.1 -- not an asteroid (will add it to exclusion list)
00:35:22.91 +49:49:47.5 -- not an asteroid (will add it to exclusion list)
00:30:52.73 +49:19:20.6 -- not an asteroid (will add it to exclusion list)
00:47:14.56 +50:21:14.0 -- not an asteroid (will add it to exclusion list)
00:45:21.83 +50:47:05.3 -- not an asteroid (will add it to exclusion list)
00:38:25.76 +49:06:31.7 -- not an asteroid (will add it to exclusion list)
00:45:52.36 +50:24:02.4 -- not an asteroid (will add it to exclusion list)
00:29:26.24 +49:15:18.3 -- not an asteroid (will add it to exclusion list)
00:46:46.22 +49:46:26.9 -- not an asteroid (will add it to exclusion list)
00:41:06.82 +49:38:11.5 -- not an asteroid (will add it to exclusion list)
00:25:46.33 +57:59:01.6 -- not an asteroid (will add it to exclusion list)
00:40:46.97 +50:18:52.3 -- not an asteroid (will add it to exclusion list)
00:47:53.87 +51:24:28.5 -- not an asteroid (will add it to exclusion list)
00:39:00.38 +49:13:32.7 -- not an asteroid (will add it to exclusion list)
00:38:51.17 +49:35:21.5 -- not an asteroid (will add it to exclusion list)
00:44:05.27 +49:44:08.0 -- not an asteroid (will add it to exclusion list)
00:38:26.79 +48:56:46.1 -- not an asteroid (will add it to exclusion list)
00:42:11.50 +50:45:53.0 -- not an asteroid (will add it to exclusion list)
00:38:58.05 +50:19:33.2 -- not an asteroid (will add it to exclusion list)
00:48:01.29 +53:47:45.1 -- not an asteroid (will add it to exclusion list)
00:44:58.37 +50:03:21.4 -- not an asteroid (will add it to exclusion list)
23:23:16.71 +52:26:44.9 -- not an asteroid (will add it to exclusion list)
00:46:51.47 +50:27:44.6 -- not an asteroid (will add it to exclusion list)
00:37:19.86 +49:22:16.7 -- not an asteroid (will add it to exclusion list)
00:45:46.68 +50:38:15.2 -- not an asteroid (will add it to exclusion list)
00:35:36.16 +49:54:16.9 -- not an asteroid (will add it to exclusion list)
00:38:59.19 +49:06:42.7 -- not an asteroid (will add it to exclusion list)
00:45:42.35 +51:05:26.9 -- not an asteroid (will add it to exclusion list)
00:41:21.50 +51:05:37.9 -- not an asteroid (will add it to exclusion list)
00:36:47.78 +49:20:39.3 -- not an asteroid (will add it to exclusion list)
00:48:36.44 +51:29:37.3 -- not an asteroid (will add it to exclusion list)
00:43:53.05 +50:11:02.3 -- not an asteroid (will add it to exclusion list)
00:43:11.52 +49:49:44.5 -- not an asteroid (will add it to exclusion list)
00:44:42.74 +49:41:44.6 -- not an asteroid (will add it to exclusion list)
00:43:09.86 +50:58:24.1 -- not an asteroid (will add it to exclusion list)
00:44:05.44 +50:43:01.4 -- not an asteroid (will add it to exclusion list)
00:29:55.38 +49:08:27.7 -- not an asteroid (will add it to exclusion list)
00:38:16.02 +50:15:21.6 -- not an asteroid (will add it to exclusion list)
00:47:41.64 +50:48:50.0 -- not an asteroid (will add it to exclusion list)
00:41:47.49 +50:16:05.0 -- not an asteroid (will add it to exclusion list)
00:47:16.25 +50:51:07.5 -- not an asteroid (will add it to exclusion list)
00:34:40.97 +49:51:06.3 -- not an asteroid (will add it to exclusion list)
00:44:26.66 +49:49:48.2 -- not an asteroid (will add it to exclusion list)
00:54:51.88 +56:45:46.4 -- not an asteroid (will add it to exclusion list)
00:49:49.28 +51:59:45.6 -- not an asteroid (will add it to exclusion list)
00:33:35.04 +48:58:44.3 -- not an asteroid (will add it to exclusion list)
00:36:32.00 +49:04:15.8 -- not an asteroid (will add it to exclusion list)
00:38:25.34 +50:36:26.1 -- not an asteroid (will add it to exclusion list)
00:34:55.96 +49:03:58.2 -- not an asteroid (will add it to exclusion list)
00:39:45.58 +48:44:26.7 -- not an asteroid (will add it to exclusion list)
23:08:57.49 +53:23:18.7 -- not an asteroid (will add it to exclusion list)
00:46:17.92 +49:55:56.4 -- not an asteroid (will add it to exclusion list)
00:41:29.60 +49:57:06.5 -- not an asteroid (will add it to exclusion list)
00:43:45.45 +50:34:56.0 -- not an asteroid (will add it to exclusion list)
00:47:07.85 +50:10:53.4 -- not an asteroid (will add it to exclusion list)
00:44:59.23 +50:13:07.3 -- not an asteroid (will add it to exclusion list)
23:35:49.76 +51:16:44.8 -- not an asteroid (will add it to exclusion list)
00:48:23.17 +54:48:53.2 -- not an asteroid (will add it to exclusion list)
00:46:00.47 +49:48:02.8 -- not an asteroid (will add it to exclusion list)
00:38:33.21 +48:51:35.5 -- not an asteroid (will add it to exclusion list)
00:29:32.59 +48:52:54.5 -- not an asteroid (will add it to exclusion list)
00:43:06.12 +50:04:43.7 -- not an asteroid (will add it to exclusion list)
00:44:09.72 +50:56:04.3 -- not an asteroid (will add it to exclusion list)
00:41:42.76 +49:30:08.8 -- not an asteroid (will add it to exclusion list)
00:32:51.73 +50:26:51.0 -- not an asteroid (will add it to exclusion list)
00:40:05.03 +49:06:39.4 -- not an asteroid (will add it to exclusion list)
00:38:46.06 +50:08:08.9 -- not an asteroid (will add it to exclusion list)
00:43:31.49 +50:48:15.7 -- not an asteroid (will add it to exclusion list)
00:43:50.67 +49:59:41.7 -- not an asteroid (will add it to exclusion list)
00:48:19.07 +50:56:33.0 -- not an asteroid (will add it to exclusion list)
00:36:40.92 +49:23:46.2 -- not an asteroid (will add it to exclusion list)
00:02:36.41 +55:35:39.4 -- not an asteroid (will add it to exclusion list)
00:43:11.46 +50:19:29.1 -- not an asteroid (will add it to exclusion list)
00:46:14.54 +50:13:40.4 -- not an asteroid (will add it to exclusion list)
00:39:37.61 +49:41:10.3 -- not an asteroid (will add it to exclusion list)
00:36:02.81 +49:16:40.5 -- not an asteroid (will add it to exclusion list)
00:43:49.95 +50:02:21.8 -- not an asteroid (will add it to exclusion list)
00:56:43.95 +57:23:36.4 -- not an asteroid (will add it to exclusion list)
00:36:35.81 +49:27:25.3 -- not an asteroid (will add it to exclusion list)
00:36:46.61 +49:32:55.0 -- not an asteroid (will add it to exclusion list)
00:41:12.81 +49:20:24.3 -- not an asteroid (will add it to exclusion list)
00:37:52.79 +49:45:39.9 -- not an asteroid (will add it to exclusion list)
00:44:04.96 +50:24:35.5 -- not an asteroid (will add it to exclusion list)
23:25:05.02 +55:05:34.3 -- not an asteroid (will add it to exclusion list)
00:41:28.09 +50:30:28.5 -- not an asteroid (will add it to exclusion list)
00:42:59.23 +50:16:22.0 -- not an asteroid (will add it to exclusion list)
00:39:41.88 +50:10:46.9 -- not an asteroid (will add it to exclusion list)
00:33:40.12 +49:45:25.6 -- not an asteroid (will add it to exclusion list)
00:50:42.09 +57:57:35.7 -- not an asteroid (will add it to exclusion list)
00:35:45.67 +49:13:52.9 -- not an asteroid (will add it to exclusion list)
00:41:29.77 +50:40:23.7 -- not an asteroid (will add it to exclusion list)
23:08:22.62 +55:49:47.2 -- not an asteroid (will add it to exclusion list)
00:42:57.24 +50:03:47.4 -- not an asteroid (will add it to exclusion list)
00:36:14.23 +49:21:55.9 -- not an asteroid (will add it to exclusion list)
00:48:48.54 +51:15:20.3 -- not an asteroid (will add it to exclusion list)
00:31:10.03 +49:14:57.5 -- not an asteroid (will add it to exclusion list)
00:36:55.44 +48:50:41.1 -- not an asteroid (will add it to exclusion list)
00:43:50.81 +49:27:00.4 -- not an asteroid (will add it to exclusion list)
00:33:05.52 +49:31:10.2 -- not an asteroid (will add it to exclusion list)
00:42:38.36 +51:09:47.4 -- not an asteroid (will add it to exclusion list)
00:43:42.89 +49:43:38.4 -- not an asteroid (will add it to exclusion list)
00:33:00.47 +49:11:35.9 -- not an asteroid (will add it to exclusion list)
00:28:15.88 +48:43:18.0 -- not an asteroid (will add it to exclusion list)
00:37:15.82 +50:03:05.3 -- not an asteroid (will add it to exclusion list)
23:49:50.08 +53:26:58.0 -- not an asteroid (will add it to exclusion list)
00:42:28.55 +49:30:37.3 -- not an asteroid (will add it to exclusion list)
00:47:33.94 +51:22:13.1 -- not an asteroid (will add it to exclusion list)
00:16:11.31 +49:15:05.4 -- not an asteroid (will add it to exclusion list)
00:40:29.52 +50:01:01.3 -- not an asteroid (will add it to exclusion list)
00:41:38.91 +50:27:39.9 -- not an asteroid (will add it to exclusion list)
00:31:56.92 +49:18:09.7 -- not an asteroid (will add it to exclusion list)
00:44:22.71 +49:48:54.5 -- not an asteroid (will add it to exclusion list)
00:37:42.99 +49:34:53.4 -- not an asteroid (will add it to exclusion list)
00:44:34.34 +50:15:23.5 -- not an asteroid (will add it to exclusion list)
00:33:38.04 +48:56:21.0 -- not an asteroid (will add it to exclusion list)
00:46:54.69 +50:39:25.0 -- not an asteroid (will add it to exclusion list)
00:43:14.24 +49:38:10.6 -- not an asteroid (will add it to exclusion list)
00:34:06.99 +49:36:32.0 -- not an asteroid (will add it to exclusion list)
00:41:52.51 +49:45:52.2 -- not an asteroid (will add it to exclusion list)
00:35:41.72 +49:31:18.6 -- not an asteroid (will add it to exclusion list)
00:38:37.19 +48:53:14.6 -- not an asteroid (will add it to exclusion list)
00:42:06.28 +50:45:22.0 -- not an asteroid (will add it to exclusion list)
00:49:00.11 +51:55:18.7 -- not an asteroid (will add it to exclusion list)
00:35:10.25 +49:13:30.4 -- not an asteroid (will add it to exclusion list)
00:45:35.04 +50:06:54.9 -- not an asteroid (will add it to exclusion list)
00:41:50.04 +50:11:56.9 -- not an asteroid (will add it to exclusion list)
00:43:26.77 +50:14:20.5 -- not an asteroid (will add it to exclusion list)
23:16:02.64 +53:58:02.4 -- not an asteroid (will add it to exclusion list)
00:44:12.55 +50:33:09.4 -- not an asteroid (will add it to exclusion list)
00:40:26.52 +49:52:04.2 -- not an asteroid (will add it to exclusion list)
00:40:17.36 +49:38:27.2 -- not an asteroid (will add it to exclusion list)
00:46:08.11 +50:17:34.9 -- not an asteroid (will add it to exclusion list)
00:36:53.34 +49:27:42.2 -- not an asteroid (will add it to exclusion list)
00:47:01.70 +50:42:52.3 -- not an asteroid (will add it to exclusion list)
00:38:01.64 +49:00:50.7 -- not an asteroid (will add it to exclusion list)
00:49:38.43 +51:51:57.0 -- not an asteroid (will add it to exclusion list)
00:47:48.94 +51:15:14.7 -- not an asteroid (will add it to exclusion list)
00:41:59.49 +49:46:29.2 -- not an asteroid (will add it to exclusion list)
00:43:19.16 +49:55:12.4 -- not an asteroid (will add it to exclusion list)
00:34:00.17 +49:37:27.3 -- not an asteroid (will add it to exclusion list)
00:46:15.15 +49:37:46.0 -- not an asteroid (will add it to exclusion list)
00:44:08.70 +49:37:08.8 -- not an asteroid (will add it to exclusion list)
00:41:18.79 +50:23:11.4 -- not an asteroid (will add it to exclusion list)
00:46:30.01 +51:10:00.8 -- not an asteroid (will add it to exclusion list)
00:46:45.82 +50:14:20.7 -- not an asteroid (will add it to exclusion list)
00:39:13.54 +49:40:17.3 -- not an asteroid (will add it to exclusion list)
00:28:11.92 +49:22:01.3 -- not an asteroid (will add it to exclusion list)
00:38:16.15 +49:02:55.2 -- not an asteroid (will add it to exclusion list)
23:29:14.19 +53:24:27.1 -- not an asteroid (will add it to exclusion list)
00:47:56.81 +51:05:58.0 -- not an asteroid (will add it to exclusion list)
00:42:02.11 +50:39:27.8 -- not an asteroid (will add it to exclusion list)
00:47:00.30 +58:07:18.8 -- not an asteroid (will add it to exclusion list)
00:37:00.43 +48:58:17.9 -- not an asteroid (will add it to exclusion list)
00:35:14.12 +50:03:26.3 -- not an asteroid (will add it to exclusion list)
00:45:54.99 +50:24:54.3 -- not an asteroid (will add it to exclusion list)
00:41:00.79 +49:46:02.8 -- not an asteroid (will add it to exclusion list)
00:37:13.07 +50:18:04.1 -- not an asteroid (will add it to exclusion list)
00:40:07.31 +50:28:21.6 -- not an asteroid (will add it to exclusion list)
00:44:56.27 +50:15:32.7 -- not an asteroid (will add it to exclusion list)
00:39:18.87 +49:31:19.9 -- not an asteroid (will add it to exclusion list)
00:29:08.31 +49:02:49.1 -- not an asteroid (will add it to exclusion list)
00:37:51.50 +49:25:31.9 -- not an asteroid (will add it to exclusion list)
00:34:37.06 +49:02:32.4 -- not an asteroid (will add it to exclusion list)
00:31:47.72 +49:24:29.2 -- not an asteroid (will add it to exclusion list)
00:46:18.71 +50:55:13.5 -- not an asteroid (will add it to exclusion list)
00:41:45.39 +49:38:15.5 -- not an asteroid (will add it to exclusion list)
00:35:42.35 +49:48:55.2 -- not an asteroid (will add it to exclusion list)
00:42:08.09 +49:34:51.3 -- not an asteroid (will add it to exclusion list)
00:30:23.86 +49:14:52.6 -- not an asteroid (will add it to exclusion list)
00:47:38.64 +51:01:39.2 -- not an asteroid (will add it to exclusion list)
00:42:11.39 +49:32:38.0 -- not an asteroid (will add it to exclusion list)
00:47:34.39 +50:57:36.5 -- not an asteroid (will add it to exclusion list)
00:43:34.41 +49:42:59.4 -- not an asteroid (will add it to exclusion list)
23:42:21.26 +57:04:54.2 -- not an asteroid (will add it to exclusion list)
00:41:20.21 +49:42:43.6 -- not an asteroid (will add it to exclusion list)
00:46:38.80 +50:30:06.2 -- not an asteroid (will add it to exclusion list)
00:41:29.89 +50:21:53.2 -- not an asteroid (will add it to exclusion list)
00:46:43.15 +49:55:58.5 -- not an asteroid (will add it to exclusion list)
00:41:55.96 +50:06:51.5 -- not an asteroid (will add it to exclusion list)
00:44:16.75 +50:19:50.6 -- not an asteroid (will add it to exclusion list)
00:43:00.03 +50:33:03.3 -- not an asteroid (will add it to exclusion list)
00:34:57.86 +49:17:03.0 -- not an asteroid (will add it to exclusion list)
00:31:58.44 +49:07:28.5 -- not an asteroid (will add it to exclusion list)
00:33:05.59 +49:06:48.4 -- not an asteroid (will add it to exclusion list)
00:36:42.33 +49:06:19.3 -- not an asteroid (will add it to exclusion list)
00:44:43.10 +50:10:15.0 -- not an asteroid (will add it to exclusion list)
00:30:19.86 +48:50:51.9 -- not an asteroid (will add it to exclusion list)
00:35:56.60 +48:58:49.7 -- not an asteroid (will add it to exclusion list)
23:33:41.18 +49:58:08.9 -- not an asteroid (will add it to exclusion list)
00:35:03.83 +50:12:02.8 -- not an asteroid (will add it to exclusion list)
00:35:50.04 +48:59:20.0 -- not an asteroid (will add it to exclusion list)
00:46:26.92 +51:18:33.0 -- not an asteroid (will add it to exclusion list)
00:33:59.40 +50:02:29.6 -- not an asteroid (will add it to exclusion list)
23:32:20.38 +54:04:39.5 -- not an asteroid (will add it to exclusion list)
00:30:06.84 +49:24:56.5 -- not an asteroid (will add it to exclusion list)
00:42:43.93 +50:52:44.5 -- not an asteroid (will add it to exclusion list)
00:38:46.94 +49:15:20.7 -- not an asteroid (will add it to exclusion list)
00:46:10.02 +50:39:38.1 -- not an asteroid (will add it to exclusion list)
00:42:52.48 +50:10:11.2 -- not an asteroid (will add it to exclusion list)
00:39:45.11 +50:27:52.4 -- not an asteroid (will add it to exclusion list)
00:36:50.92 +49:58:17.1 -- not an asteroid (will add it to exclusion list)
00:40:09.34 +49:54:02.9 -- not an asteroid (will add it to exclusion list)
00:45:36.48 +50:15:29.1 -- not an asteroid (will add it to exclusion list)
00:33:35.61 +49:08:21.9 -- not an asteroid (will add it to exclusion list)
00:43:54.83 +49:43:20.1 -- not an asteroid (will add it to exclusion list)
00:45:25.13 +51:00:06.9 -- not an asteroid (will add it to exclusion list)
00:36:02.94 +49:22:20.1 -- not an asteroid (will add it to exclusion list)
00:34:11.17 +49:07:20.9 -- not an asteroid (will add it to exclusion list)
00:46:39.22 +51:36:36.2 -- not an asteroid (will add it to exclusion list)
00:29:47.99 +49:19:48.4 -- not an asteroid (will add it to exclusion list)
00:35:06.30 +49:53:43.8 -- not an asteroid (will add it to exclusion list)
00:40:28.12 +50:15:58.0 -- not an asteroid (will add it to exclusion list)
00:36:12.15 +49:57:42.5 -- not an asteroid (will add it to exclusion list)
23:33:31.05 +52:42:15.6 -- not an asteroid (will add it to exclusion list)
00:33:31.39 +50:04:38.4 -- not an asteroid (will add it to exclusion list)
00:41:50.21 +50:26:18.5 -- not an asteroid (will add it to exclusion list)
00:28:14.13 +48:45:48.1 -- not an asteroid (will add it to exclusion list)
00:40:03.09 +48:49:47.8 -- not an asteroid (will add it to exclusion list)
00:44:45.05 +49:44:26.1 -- not an asteroid (will add it to exclusion list)
00:37:58.58 +49:59:06.2 -- not an asteroid (will add it to exclusion list)
00:46:09.87 +51:24:24.0 -- not an asteroid (will add it to exclusion list)
00:42:09.50 +50:18:51.6 -- not an asteroid (will add it to exclusion list)
00:41:07.40 +50:43:02.2 -- not an asteroid (will add it to exclusion list)
00:35:22.89 +49:14:54.1 -- not an asteroid (will add it to exclusion list)
00:31:28.00 +49:10:51.3 -- not an asteroid (will add it to exclusion list)
00:38:26.44 +50:13:43.8 -- not an asteroid (will add it to exclusion list)
00:33:11.13 +49:10:15.8 -- not an asteroid (will add it to exclusion list)
00:43:40.88 +49:57:32.0 -- not an asteroid (will add it to exclusion list)
00:45:01.41 +50:21:07.3 -- not an asteroid (will add it to exclusion list)
00:36:24.46 +50:09:02.1 -- not an asteroid (will add it to exclusion list)
00:45:08.56 +50:23:58.5 -- not an asteroid (will add it to exclusion list)
23:38:36.59 +57:11:43.8 -- not an asteroid (will add it to exclusion list)
00:44:37.90 +50:16:26.2 -- not an asteroid (will add it to exclusion list)
00:34:04.89 +49:39:52.6 -- not an asteroid (will add it to exclusion list)
00:45:43.06 +51:24:41.2 -- not an asteroid (will add it to exclusion list)
00:42:00.00 +49:31:12.7 -- not an asteroid (will add it to exclusion list)
23:25:30.77 +57:09:53.7 -- not an asteroid (will add it to exclusion list)
00:34:44.60 +49:41:17.9 -- not an asteroid (will add it to exclusion list)
00:30:19.81 +48:56:58.7 -- not an asteroid (will add it to exclusion list)
23:24:32.34 +57:07:12.4 -- not an asteroid (will add it to exclusion list)
00:39:21.14 +50:28:23.6 -- not an asteroid (will add it to exclusion list)
00:45:50.71 +50:35:01.8 -- not an asteroid (will add it to exclusion list)
00:41:27.08 +50:23:44.8 -- not an asteroid (will add it to exclusion list)
00:40:29.75 +49:05:50.1 -- not an asteroid (will add it to exclusion list)
00:43:25.12 +50:19:24.6 -- not an asteroid (will add it to exclusion list)
00:41:25.86 +49:49:30.6 -- not an asteroid (will add it to exclusion list)
00:42:02.89 +49:45:10.8 -- not an asteroid (will add it to exclusion list)
00:33:40.47 +49:11:41.2 -- not an asteroid (will add it to exclusion list)
00:36:35.35 +49:51:39.6 -- not an asteroid (will add it to exclusion list)
00:48:02.49 +51:33:32.7 -- not an asteroid (will add it to exclusion list)
00:47:02.28 +50:32:18.5 -- not an asteroid (will add it to exclusion list)
00:38:35.35 +48:55:17.9 -- not an asteroid (will add it to exclusion list)
00:38:29.97 +50:26:20.4 -- not an asteroid (will add it to exclusion list)
00:28:30.56 +49:04:19.4 -- not an asteroid (will add it to exclusion list)
00:12:08.83 +50:38:18.1 -- not an asteroid (will add it to exclusion list)
00:29:50.13 +48:49:10.3 -- not an asteroid (will add it to exclusion list)
00:30:50.84 +49:58:09.9 -- not an asteroid (will add it to exclusion list)
00:45:56.19 +51:22:51.1 -- not an asteroid (will add it to exclusion list)
00:43:44.44 +51:06:54.1 -- not an asteroid (will add it to exclusion list)
00:55:31.18 +56:33:11.6 -- not an asteroid (will add it to exclusion list)
23:57:50.00 +56:34:46.4 -- not an asteroid (will add it to exclusion list)
00:53:12.38 +54:48:07.2 -- not an asteroid (will add it to exclusion list)
00:44:39.41 +51:41:05.1 -- not an asteroid (will add it to exclusion list)
00:48:55.16 +53:00:35.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:02:36.41 +55:35:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:11.16 +57:55:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:08.83 +50:38:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:11.31 +49:15:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:03.08 +55:19:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:46.33 +57:59:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:50.36 +49:10:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:08.02 +48:44:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:20.86 +48:44:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:32.28 +48:49:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:48.38 +48:44:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:11.92 +49:22:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:14.13 +48:45:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:15.88 +48:43:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:30.56 +49:04:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:08.31 +49:02:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:26.24 +49:15:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:32.59 +48:52:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:36.60 +48:56:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:36.73 +48:43:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:41.61 +48:41:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:47.99 +49:19:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:48.44 +49:15:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:50.13 +48:49:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:53.01 +50:05:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:53.36 +50:13:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:55.38 +49:08:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:55.57 +49:08:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:06.84 +49:24:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:09.45 +49:34:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:09.72 +49:12:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:19.81 +48:56:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:19.86 +48:50:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:23.39 +48:54:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:23.86 +49:14:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:29.22 +55:18:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:37.49 +49:15:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:43.92 +49:15:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:50.84 +49:58:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:52.73 +49:19:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:54.04 +49:16:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:57.89 +49:16:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:10.03 +49:14:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:10.05 +55:39:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:24.77 +49:05:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:28.00 +49:10:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:30.22 +49:04:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:33.33 +49:18:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:47.72 +49:24:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:51.19 +49:28:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:56.92 +49:18:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:58.44 +49:07:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:59.22 +49:09:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:01.16 +49:19:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:20.07 +49:32:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:49.72 +49:11:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:51.73 +50:26:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:51.85 +49:19:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:52.96 +48:59:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:00.47 +49:11:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:00.64 +49:33:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:05.52 +49:31:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:05.59 +49:06:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:05.91 +49:26:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:07.73 +49:00:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:11.13 +49:10:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:15.80 +49:05:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:18.41 +49:37:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:26.77 +49:19:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:31.39 +50:04:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:35.04 +48:58:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:35.61 +49:08:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:37.46 +49:04:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:38.04 +48:56:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:40.12 +49:45:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:40.47 +49:11:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:46.17 +49:46:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:51.13 +49:19:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:59.40 +50:02:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:00.17 +49:37:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:01.04 +49:25:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:02.57 +49:31:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:03.66 +49:02:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:04.42 +49:01:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:04.89 +49:39:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:06.99 +49:36:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:08.69 +48:55:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:11.17 +49:07:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:16.96 +49:38:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:22.76 +49:57:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:23.47 +49:51:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:23.57 +49:19:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:24.15 +49:22:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:29.49 +49:19:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:30.75 +49:44:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:32.63 +48:57:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:33.44 +49:23:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:35.21 +49:51:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:35.94 +49:33:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:36.11 +49:29:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:37.06 +49:02:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:40.16 +48:54:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:40.93 +49:36:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:40.97 +49:51:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:43.02 +49:42:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:44.60 +49:41:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:49.24 +49:02:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:52.01 +49:01:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:55.96 +49:03:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:56.95 +48:53:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:57.81 +49:53:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:57.86 +49:17:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:03.83 +50:12:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:06.30 +49:53:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:09.45 +49:16:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:09.93 +49:02:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:10.25 +49:13:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:14.12 +50:03:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:17.56 +49:14:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:22.89 +49:14:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:22.91 +49:49:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:23.59 +49:04:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:36.16 +49:54:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:41.72 +49:31:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:42.35 +49:48:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:45.67 +49:13:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:46.59 +49:23:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:46.91 +49:26:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:50.04 +48:59:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:56.60 +48:58:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:02.81 +49:16:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:02.94 +49:22:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:12.15 +49:57:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:14.23 +49:21:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:24.00 +49:29:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:24.46 +50:09:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:30.32 +49:32:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:32.00 +49:04:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:35.35 +49:51:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:35.64 +49:09:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:35.81 +49:27:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:40.92 +49:23:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:42.33 +49:06:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:46.61 +49:32:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:47.78 +49:20:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:50.92 +49:58:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:53.34 +49:27:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:55.44 +48:50:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:00.43 +48:58:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:06.77 +48:54:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:13.07 +50:18:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:15.82 +50:03:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:19.86 +49:22:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:42.99 +49:34:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:47.79 +49:14:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:51.50 +49:25:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:52.79 +49:45:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:58.58 +49:59:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:01.64 +49:00:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:16.02 +50:15:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:16.15 +49:02:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:16.91 +49:08:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:19.01 +49:03:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:25.34 +50:36:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:25.76 +49:06:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:26.44 +50:13:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:26.79 +48:56:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:29.97 +50:26:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:30.74 +49:12:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:33.21 +48:51:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:35.35 +48:55:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:37.19 +48:53:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:46.06 +50:08:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:46.94 +49:15:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:51.17 +49:35:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:58.05 +50:19:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:59.19 +49:06:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:00.38 +49:13:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:01.48 +49:30:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:11.60 +50:29:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:11.67 +49:08:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:13.54 +49:40:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:17.09 +49:07:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:17.65 +49:05:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:18.87 +49:31:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:21.14 +50:28:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:23.37 +48:58:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:33.86 +49:10:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:34.85 +48:54:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:35.16 +48:51:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:37.61 +49:41:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:37.63 +49:24:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:40.72 +49:07:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:41.88 +50:10:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:42.16 +49:10:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:45.11 +50:27:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:45.58 +48:44:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:56.30 +49:02:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:03.09 +48:49:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:05.03 +49:06:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:07.31 +50:28:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:09.34 +49:54:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:17.36 +49:38:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:24.89 +49:16:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:26.52 +49:52:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:28.12 +50:15:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:29.52 +50:01:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:29.75 +49:05:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:46.97 +50:18:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:58.27 +48:54:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:00.79 +49:46:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:06.82 +49:38:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:07.40 +50:43:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:12.81 +49:20:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:18.79 +50:23:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:20.21 +49:42:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:21.50 +51:05:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:25.86 +49:49:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:27.08 +50:23:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:28.09 +50:30:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:29.60 +49:57:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:29.77 +50:40:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:29.89 +50:21:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:38.91 +50:27:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:42.76 +49:30:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:44.34 +49:24:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:45.39 +49:38:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:47.49 +50:16:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:50.04 +50:11:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:50.21 +50:26:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:52.51 +49:45:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:55.96 +50:06:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:59.49 +49:46:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:00.00 +49:31:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:00.91 +50:58:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:02.11 +50:39:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:02.89 +49:45:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:06.28 +50:45:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:08.09 +49:34:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:09.50 +50:18:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:11.39 +49:32:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:11.50 +50:45:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:28.55 +49:30:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:29.35 +50:06:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:30.77 +50:54:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:34.61 +50:13:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:38.36 +51:09:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:43.93 +50:52:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:49.44 +50:06:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:52.48 +50:10:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:52.90 +52:06:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:54.09 +50:11:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:56.93 +50:54:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:57.24 +50:03:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:59.23 +50:16:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:59.78 +51:05:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:00.03 +50:33:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:05.25 +51:03:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:06.12 +50:04:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:09.86 +50:58:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:11.46 +50:19:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:11.52 +49:49:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:14.24 +49:38:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:16.28 +49:08:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:19.16 +49:55:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:19.98 +58:08:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:25.12 +50:19:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:26.77 +50:14:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:31.49 +50:48:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:34.41 +49:42:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:40.88 +49:57:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:42.89 +49:43:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:44.44 +51:06:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:45.45 +50:34:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:48.42 +51:02:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:49.95 +50:02:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:50.67 +49:59:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:50.81 +49:27:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:53.05 +50:11:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:54.83 +49:43:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:57.38 +51:14:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:58.21 +49:10:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:04.93 +49:03:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:04.96 +50:24:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:05.27 +49:44:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:05.44 +50:43:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:08.70 +49:37:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:09.72 +50:56:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:12.55 +50:33:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:16.75 +50:19:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:22.71 +49:48:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:26.66 +49:49:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:27.71 +50:58:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:29.36 +50:13:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:34.34 +50:15:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:37.90 +50:16:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:39.41 +51:41:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:42.74 +49:41:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:43.10 +50:10:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:43.93 +49:42:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:45.05 +49:44:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:46.84 +50:46:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:56.27 +50:15:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:58.37 +50:03:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:59.23 +50:13:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:01.41 +50:21:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:08.56 +50:23:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:21.83 +50:47:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:25.13 +51:00:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:27.46 +50:43:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:30.28 +49:28:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:35.04 +50:06:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:35.72 +50:31:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:36.48 +50:15:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:42.35 +51:05:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:43.06 +51:24:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:44.72 +49:39:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:46.68 +50:38:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:50.71 +50:35:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:52.36 +50:24:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:52.74 +50:50:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:54.99 +50:24:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:56.19 +51:22:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:56.32 +51:07:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:00.47 +49:48:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:04.86 +49:37:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:08.11 +50:17:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:09.87 +51:24:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:10.02 +50:39:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:11.97 +50:44:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:14.54 +50:13:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:15.15 +49:37:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:17.92 +49:55:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:18.32 +50:52:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:18.71 +50:55:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:23.97 +49:40:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:26.92 +51:18:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:30.01 +51:10:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:31.50 +51:13:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:38.70 +50:41:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:38.80 +50:30:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:39.22 +51:36:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:43.15 +49:55:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:45.82 +50:14:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:46.22 +49:46:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:47.03 +51:14:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:48.49 +58:10:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:51.47 +50:27:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:53.36 +50:47:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:53.59 +49:51:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:54.69 +50:39:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:00.30 +58:07:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:01.14 +51:22:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:01.70 +50:42:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:02.28 +50:32:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:07.85 +50:10:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:14.56 +50:21:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:16.25 +50:51:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:24.18 +50:34:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:33.94 +51:22:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:34.39 +50:57:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:37.20 +50:24:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:38.64 +51:01:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:41.64 +50:48:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:41.69 +50:47:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:47.57 +50:59:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:48.52 +50:46:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:48.94 +51:15:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:50.76 +51:30:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:53.87 +51:24:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:56.81 +51:05:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:01.29 +53:47:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:02.30 +50:47:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:02.49 +51:33:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:11.86 +50:59:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:12.06 +50:51:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:19.07 +50:56:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:23.17 +54:48:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:36.44 +51:29:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:47.12 +51:11:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:48.54 +51:15:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:55.16 +53:00:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:00.11 +51:55:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:38.43 +51:51:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:49.28 +51:59:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:42.09 +57:57:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:07.27 +54:59:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:12.38 +54:48:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:51.88 +56:45:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:31.18 +56:33:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:43.95 +57:23:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:52.48 +57:23:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:24.04 +57:00:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:22.62 +55:49:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:57.49 +53:23:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:51.78 +54:50:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:31.33 +56:01:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:02.64 +53:58:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:48.80 +55:26:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:32.89 +51:47:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:45.39 +53:43:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:16.71 +52:26:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:32.34 +57:07:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:05.02 +55:05:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:30.77 +57:09:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:31.85 +53:36:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:14.19 +53:24:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:09.43 +54:16:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:45.01 +54:09:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:20.38 +54:04:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:31.05 +52:42:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:41.18 +49:58:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:49.76 +51:16:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:42.81 +52:12:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:10.97 +52:49:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:36.59 +57:11:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:21.26 +57:04:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:50.08 +53:26:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:50.00 +56:34:46.4 -- 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)
00:02:36.41 +55:35:39.4 -- a known variable star
00:04:11.16 +57:55:53.2 -- not a known variable star
00:12:08.83 +50:38:18.1 -- not a known variable star
00:16:11.31 +49:15:05.4 -- not a known variable star
00:25:03.08 +55:19:43.6 -- a known variable star
00:25:46.33 +57:59:01.6 -- not a known variable star
00:26:50.36 +49:10:19.8 -- a known variable star
00:27:08.02 +48:44:41.6 -- not a known variable star
00:27:20.86 +48:44:02.2 -- not a known variable star
00:27:32.28 +48:49:11.3 -- not a known variable star
00:27:48.38 +48:44:52.3 -- not a known variable star
00:28:11.92 +49:22:01.3 -- a known variable star
00:28:14.13 +48:45:48.1 -- not a known variable star
00:28:15.88 +48:43:18.0 -- not a known variable star
00:28:30.56 +49:04:19.4 -- not a known variable star
00:29:08.31 +49:02:49.1 -- not a known variable star
00:29:26.24 +49:15:18.3 -- not a known variable star
00:29:32.59 +48:52:54.5 -- not a known variable star
00:29:36.60 +48:56:00.8 -- not a known variable star
00:29:36.73 +48:43:49.9 -- not a known variable star
00:29:41.61 +48:41:39.6 -- not a known variable star
00:29:47.99 +49:19:48.4 -- not a known variable star
00:29:48.44 +49:15:04.0 -- a known variable star
00:29:50.13 +48:49:10.3 -- not a known variable star
00:29:53.01 +50:05:46.7 -- not a known variable star
00:29:53.36 +50:13:53.1 -- not a known variable star
00:29:55.38 +49:08:27.7 -- not a known variable star
00:29:55.57 +49:08:55.6 -- not a known variable star
00:30:06.84 +49:24:56.5 -- not a known variable star
00:30:09.45 +49:34:50.7 -- not a known variable star
00:30:09.72 +49:12:21.9 -- not a known variable star
00:30:19.81 +48:56:58.7 -- not a known variable star
00:30:19.86 +48:50:51.9 -- not a known variable star
00:30:23.39 +48:54:32.5 -- not a known variable star
00:30:23.86 +49:14:52.6 -- not a known variable star
00:30:29.22 +55:18:05.8 -- not a known variable star
00:30:37.49 +49:15:38.7 -- not a known variable star
00:30:43.92 +49:15:29.0 -- not a known variable star
00:30:50.84 +49:58:09.9 -- not a known variable star
00:30:52.73 +49:19:20.6 -- not a known variable star
00:30:54.04 +49:16:44.7 -- not a known variable star
00:30:57.89 +49:16:02.0 -- not a known variable star
00:31:10.03 +49:14:57.5 -- not a known variable star
00:31:10.05 +55:39:13.7 -- not a known variable star
00:31:24.77 +49:05:00.4 -- a known variable star
00:31:28.00 +49:10:51.3 -- not a known variable star
00:31:30.22 +49:04:17.1 -- a known variable star
00:31:33.33 +49:18:21.9 -- not a known variable star
00:31:47.72 +49:24:29.2 -- a known variable star
00:31:51.19 +49:28:31.3 -- not a known variable star
00:31:56.92 +49:18:09.7 -- not a known variable star
00:31:58.44 +49:07:28.5 -- not a known variable star
00:31:59.22 +49:09:55.8 -- a known variable star
00:32:01.16 +49:19:09.0 -- not a known variable star
00:32:20.07 +49:32:47.4 -- not a known variable star
00:32:49.72 +49:11:25.7 -- not a known variable star
00:32:51.73 +50:26:51.0 -- not a known variable star
00:32:51.85 +49:19:38.8 -- a known variable star
00:32:52.96 +48:59:29.8 -- not a known variable star
00:33:00.47 +49:11:35.9 -- not a known variable star
00:33:00.64 +49:33:16.6 -- not a known variable star
00:33:05.52 +49:31:10.2 -- not a known variable star
00:33:05.59 +49:06:48.4 -- not a known variable star
00:33:05.91 +49:26:24.6 -- a known variable star
00:33:07.73 +49:00:57.2 -- not a known variable star
00:33:11.13 +49:10:15.8 -- not a known variable star
00:33:15.80 +49:05:57.8 -- not a known variable star
00:33:18.41 +49:37:35.2 -- not a known variable star
00:33:26.77 +49:19:04.2 -- not a known variable star
00:33:31.39 +50:04:38.4 -- a known variable star
00:33:35.04 +48:58:44.3 -- not a known variable star
00:33:35.61 +49:08:21.9 -- not a known variable star
00:33:37.46 +49:04:29.0 -- not a known variable star
00:33:38.04 +48:56:21.0 -- not a known variable star
00:33:40.12 +49:45:25.6 -- not a known variable star
00:33:40.47 +49:11:41.2 -- not a known variable star
00:33:46.17 +49:46:08.2 -- not a known variable star
00:33:51.13 +49:19:04.6 -- not a known variable star
00:33:59.40 +50:02:29.6 -- not a known variable star
00:34:00.17 +49:37:27.3 -- not a known variable star
00:34:01.04 +49:25:53.0 -- not a known variable star
00:34:02.57 +49:31:15.8 -- not a known variable star
00:34:03.66 +49:02:32.9 -- not a known variable star
00:34:04.42 +49:01:31.6 -- not a known variable star
00:34:04.89 +49:39:52.6 -- not a known variable star
00:34:06.99 +49:36:32.0 -- not a known variable star
00:34:08.69 +48:55:40.6 -- not a known variable star
00:34:11.17 +49:07:20.9 -- not a known variable star
00:34:16.96 +49:38:26.3 -- not a known variable star
00:34:22.76 +49:57:18.7 -- not a known variable star
00:34:23.47 +49:51:01.4 -- not a known variable star
00:34:23.57 +49:19:33.0 -- not a known variable star
00:34:24.15 +49:22:46.1 -- not a known variable star
00:34:29.49 +49:19:02.2 -- not a known variable star
00:34:30.75 +49:44:36.9 -- not a known variable star
00:34:32.63 +48:57:00.3 -- not a known variable star
00:34:33.44 +49:23:40.3 -- not a known variable star
00:34:35.21 +49:51:37.2 -- not a known variable star
00:34:35.94 +49:33:31.0 -- not a known variable star
00:34:36.11 +49:29:11.0 -- not a known variable star
00:34:37.06 +49:02:32.4 -- not a known variable star
00:34:40.16 +48:54:44.3 -- a known variable star
00:34:40.93 +49:36:47.7 -- not a known variable star
00:34:40.97 +49:51:06.3 -- not a known variable star
00:34:43.02 +49:42:52.9 -- not a known variable star
00:34:44.60 +49:41:17.9 -- not a known variable star
00:34:49.24 +49:02:01.6 -- not a known variable star
00:34:52.01 +49:01:28.4 -- not a known variable star
00:34:55.96 +49:03:58.2 -- not a known variable star
00:34:56.95 +48:53:46.8 -- not a known variable star
00:34:57.81 +49:53:58.7 -- not a known variable star
00:34:57.86 +49:17:03.0 -- not a known variable star
00:35:03.83 +50:12:02.8 -- not a known variable star
00:35:06.30 +49:53:43.8 -- not a known variable star
00:35:09.45 +49:16:34.4 -- not a known variable star
00:35:09.93 +49:02:17.0 -- a known variable star
00:35:10.25 +49:13:30.4 -- a known variable star
00:35:14.12 +50:03:26.3 -- a known variable star
00:35:17.56 +49:14:23.8 -- a known variable star
00:35:22.89 +49:14:54.1 -- not a known variable star
00:35:22.91 +49:49:47.5 -- not a known variable star
00:35:23.59 +49:04:22.7 -- not a known variable star
00:35:36.16 +49:54:16.9 -- not a known variable star
00:35:41.72 +49:31:18.6 -- a known variable star
00:35:42.35 +49:48:55.2 -- a known variable star
00:35:45.67 +49:13:52.9 -- not a known variable star
00:35:46.59 +49:23:09.7 -- not a known variable star
00:35:46.91 +49:26:55.0 -- not a known variable star
00:35:50.04 +48:59:20.0 -- not a known variable star
00:35:56.60 +48:58:49.7 -- not a known variable star
00:36:02.81 +49:16:40.5 -- not a known variable star
00:36:02.94 +49:22:20.1 -- not a known variable star
00:36:12.15 +49:57:42.5 -- a known variable star
00:36:14.23 +49:21:55.9 -- not a known variable star
00:36:24.00 +49:29:18.0 -- not a known variable star
00:36:24.46 +50:09:02.1 -- not a known variable star
00:36:30.32 +49:32:05.3 -- not a known variable star
00:36:32.00 +49:04:15.8 -- not a known variable star
00:36:35.35 +49:51:39.6 -- not a known variable star
00:36:35.64 +49:09:00.6 -- a known variable star
00:36:35.81 +49:27:25.3 -- not a known variable star
00:36:40.92 +49:23:46.2 -- not a known variable star
00:36:42.33 +49:06:19.3 -- not a known variable star
00:36:46.61 +49:32:55.0 -- not a known variable star
00:36:47.78 +49:20:39.3 -- a known variable star
00:36:50.92 +49:58:17.1 -- not a known variable star
00:36:53.34 +49:27:42.2 -- not a known variable star
00:36:55.44 +48:50:41.1 -- not a known variable star
00:37:00.43 +48:58:17.9 -- not a known variable star
00:37:06.77 +48:54:59.7 -- not a known variable star
00:37:13.07 +50:18:04.1 -- not a known variable star
00:37:15.82 +50:03:05.3 -- not a known variable star
00:37:19.86 +49:22:16.7 -- not a known variable star
00:37:42.99 +49:34:53.4 -- a known variable star
00:37:47.79 +49:14:14.2 -- not a known variable star
00:37:51.50 +49:25:31.9 -- not a known variable star
00:37:52.79 +49:45:39.9 -- not a known variable star
00:37:58.58 +49:59:06.2 -- not a known variable star
00:38:01.64 +49:00:50.7 -- not a known variable star
00:38:16.02 +50:15:21.6 -- not a known variable star
00:38:16.15 +49:02:55.2 -- a known variable star
00:38:16.91 +49:08:28.6 -- a known variable star
00:38:19.01 +49:03:44.9 -- not a known variable star
00:38:25.34 +50:36:26.1 -- a known variable star
00:38:25.76 +49:06:31.7 -- not a known variable star
00:38:26.44 +50:13:43.8 -- not a known variable star
00:38:26.79 +48:56:46.1 -- not a known variable star
00:38:29.97 +50:26:20.4 -- not a known variable star
00:38:30.74 +49:12:54.0 -- a known variable star
00:38:33.21 +48:51:35.5 -- not a known variable star
00:38:35.35 +48:55:17.9 -- not a known variable star
00:38:37.19 +48:53:14.6 -- not a known variable star
00:38:46.06 +50:08:08.9 -- not a known variable star
00:38:46.94 +49:15:20.7 -- not a known variable star
00:38:51.17 +49:35:21.5 -- not a known variable star
00:38:58.05 +50:19:33.2 -- not a known variable star
00:38:59.19 +49:06:42.7 -- not a known variable star
00:39:00.38 +49:13:32.7 -- not a known variable star
00:39:01.48 +49:30:16.9 -- not a known variable star
00:39:11.60 +50:29:50.6 -- not a known variable star
00:39:11.67 +49:08:18.6 -- not a known variable star
00:39:13.54 +49:40:17.3 -- not a known variable star
00:39:17.09 +49:07:03.5 -- not a known variable star
00:39:17.65 +49:05:13.0 -- not a known variable star
00:39:18.87 +49:31:19.9 -- not a known variable star
00:39:21.14 +50:28:23.6 -- a known variable star
00:39:23.37 +48:58:48.7 -- a known variable star
00:39:33.86 +49:10:19.8 -- a known variable star
00:39:34.85 +48:54:30.4 -- not a known variable star
00:39:35.16 +48:51:40.5 -- not a known variable star
00:39:37.61 +49:41:10.3 -- not a known variable star
00:39:37.63 +49:24:22.0 -- not a known variable star
00:39:40.72 +49:07:27.9 -- not a known variable star
00:39:41.88 +50:10:46.9 -- not a known variable star
00:39:42.16 +49:10:15.2 -- not a known variable star
00:39:45.11 +50:27:52.4 -- not a known variable star
00:39:45.58 +48:44:26.7 -- a known variable star
00:39:56.30 +49:02:10.3 -- not a known variable star
00:40:03.09 +48:49:47.8 -- not a known variable star
00:40:05.03 +49:06:39.4 -- not a known variable star
00:40:07.31 +50:28:21.6 -- not a known variable star
00:40:09.34 +49:54:02.9 -- not a known variable star
00:40:17.36 +49:38:27.2 -- not a known variable star
00:40:24.89 +49:16:21.4 -- not a known variable star
00:40:26.52 +49:52:04.2 -- not a known variable star
00:40:28.12 +50:15:58.0 -- not a known variable star
00:40:29.52 +50:01:01.3 -- not a known variable star
00:40:29.75 +49:05:50.1 -- not a known variable star
00:40:46.97 +50:18:52.3 -- not a known variable star
00:40:58.27 +48:54:05.6 -- not a known variable star
00:41:00.79 +49:46:02.8 -- not a known variable star
00:41:06.82 +49:38:11.5 -- not a known variable star
00:41:07.40 +50:43:02.2 -- not a known variable star
00:41:12.81 +49:20:24.3 -- not a known variable star
00:41:18.79 +50:23:11.4 -- a known variable star
00:41:20.21 +49:42:43.6 -- not a known variable star
00:41:21.50 +51:05:37.9 -- not a known variable star
00:41:25.86 +49:49:30.6 -- not a known variable star
00:41:27.08 +50:23:44.8 -- not a known variable star
00:41:28.09 +50:30:28.5 -- not a known variable star
00:41:29.60 +49:57:06.5 -- not a known variable star
00:41:29.77 +50:40:23.7 -- not a known variable star
00:41:29.89 +50:21:53.2 -- not a known variable star
00:41:38.91 +50:27:39.9 -- a known variable star
00:41:42.76 +49:30:08.8 -- not a known variable star
00:41:44.34 +49:24:11.3 -- not a known variable star
00:41:45.39 +49:38:15.5 -- not a known variable star
00:41:47.49 +50:16:05.0 -- not a known variable star
00:41:50.04 +50:11:56.9 -- not a known variable star
00:41:50.21 +50:26:18.5 -- not a known variable star
00:41:52.51 +49:45:52.2 -- not a known variable star
00:41:55.96 +50:06:51.5 -- not a known variable star
00:41:59.49 +49:46:29.2 -- not a known variable star
00:42:00.00 +49:31:12.7 -- not a known variable star
00:42:00.91 +50:58:01.7 -- not a known variable star
00:42:02.11 +50:39:27.8 -- a known variable star
00:42:02.89 +49:45:10.8 -- not a known variable star
00:42:06.28 +50:45:22.0 -- not a known variable star
00:42:08.09 +49:34:51.3 -- a known variable star
00:42:09.50 +50:18:51.6 -- not a known variable star
00:42:11.39 +49:32:38.0 -- not a known variable star
00:42:11.50 +50:45:53.0 -- not a known variable star
00:42:28.55 +49:30:37.3 -- not a known variable star
00:42:29.35 +50:06:33.1 -- not a known variable star
00:42:30.77 +50:54:50.5 -- not a known variable star
00:42:34.61 +50:13:17.7 -- not a known variable star
00:42:38.36 +51:09:47.4 -- not a known variable star
00:42:43.93 +50:52:44.5 -- a known variable star
00:42:49.44 +50:06:14.3 -- not a known variable star
00:42:52.48 +50:10:11.2 -- not a known variable star
00:42:52.90 +52:06:34.0 -- not a known variable star
00:42:54.09 +50:11:16.8 -- not a known variable star
00:42:56.93 +50:54:49.2 -- not a known variable star
00:42:57.24 +50:03:47.4 -- not a known variable star
00:42:59.23 +50:16:22.0 -- not a known variable star
00:42:59.78 +51:05:48.6 -- not a known variable star
00:43:00.03 +50:33:03.3 -- not a known variable star
00:43:05.25 +51:03:48.0 -- not a known variable star
00:43:06.12 +50:04:43.7 -- not a known variable star
00:43:09.86 +50:58:24.1 -- not a known variable star
00:43:11.46 +50:19:29.1 -- not a known variable star
00:43:11.52 +49:49:44.5 -- not a known variable star
00:43:14.24 +49:38:10.6 -- not a known variable star
00:43:16.28 +49:08:58.6 -- not a known variable star
00:43:19.16 +49:55:12.4 -- not a known variable star
00:43:19.98 +58:08:06.2 -- not a known variable star
00:43:25.12 +50:19:24.6 -- not a known variable star
00:43:26.77 +50:14:20.5 -- not a known variable star
00:43:31.49 +50:48:15.7 -- not a known variable star
00:43:34.41 +49:42:59.4 -- a known variable star
00:43:40.88 +49:57:32.0 -- a known variable star
00:43:42.89 +49:43:38.4 -- not a known variable star
00:43:44.44 +51:06:54.1 -- not a known variable star
00:43:45.45 +50:34:56.0 -- a known variable star
00:43:48.42 +51:02:28.2 -- not a known variable star
00:43:49.95 +50:02:21.8 -- not a known variable star
00:43:50.67 +49:59:41.7 -- not a known variable star
00:43:50.81 +49:27:00.4 -- not a known variable star
00:43:53.05 +50:11:02.3 -- not a known variable star
00:43:54.83 +49:43:20.1 -- a known variable star
00:43:57.38 +51:14:00.1 -- a known variable star
00:43:58.21 +49:10:33.6 -- a known variable star
00:44:04.93 +49:03:55.9 -- not a known variable star
00:44:04.96 +50:24:35.5 -- not a known variable star
00:44:05.27 +49:44:08.0 -- not a known variable star
00:44:05.44 +50:43:01.4 -- not a known variable star
00:44:08.70 +49:37:08.8 -- not a known variable star
00:44:09.72 +50:56:04.3 -- not a known variable star
00:44:12.55 +50:33:09.4 -- a known variable star
00:44:16.75 +50:19:50.6 -- not a known variable star
00:44:22.71 +49:48:54.5 -- not a known variable star
00:44:26.66 +49:49:48.2 -- not a known variable star
00:44:27.71 +50:58:49.6 -- a known variable star
00:44:29.36 +50:13:55.6 -- a known variable star
00:44:34.34 +50:15:23.5 -- not a known variable star
00:44:37.90 +50:16:26.2 -- not a known variable star
00:44:39.41 +51:41:05.1 -- not a known variable star
00:44:42.74 +49:41:44.6 -- not a known variable star
00:44:43.10 +50:10:15.0 -- not a known variable star
00:44:43.93 +49:42:46.0 -- not a known variable star
00:44:45.05 +49:44:26.1 -- not a known variable star
00:44:46.84 +50:46:19.3 -- not a known variable star
00:44:56.27 +50:15:32.7 -- not a known variable star
00:44:58.37 +50:03:21.4 -- not a known variable star
00:44:59.23 +50:13:07.3 -- not a known variable star
00:45:01.41 +50:21:07.3 -- not a known variable star
00:45:08.56 +50:23:58.5 -- not a known variable star
00:45:21.83 +50:47:05.3 -- a known variable star
00:45:25.13 +51:00:06.9 -- not a known variable star
00:45:27.46 +50:43:41.0 -- not a known variable star
00:45:30.28 +49:28:32.1 -- not a known variable star
00:45:35.04 +50:06:54.9 -- not a known variable star
00:45:35.72 +50:31:49.7 -- not a known variable star
00:45:36.48 +50:15:29.1 -- a known variable star
00:45:42.35 +51:05:26.9 -- not a known variable star
00:45:43.06 +51:24:41.2 -- not a known variable star
00:45:44.72 +49:39:24.3 -- not a known variable star
00:45:46.68 +50:38:15.2 -- not a known variable star
00:45:50.71 +50:35:01.8 -- not a known variable star
00:45:52.36 +50:24:02.4 -- not a known variable star
00:45:52.74 +50:50:45.3 -- not a known variable star
00:45:54.99 +50:24:54.3 -- not a known variable star
00:45:56.19 +51:22:51.1 -- not a known variable star
00:45:56.32 +51:07:56.6 -- not a known variable star
00:46:00.47 +49:48:02.8 -- not a known variable star
00:46:04.86 +49:37:41.0 -- not a known variable star
00:46:08.11 +50:17:34.9 -- not a known variable star
00:46:09.87 +51:24:24.0 -- a known variable star
00:46:10.02 +50:39:38.1 -- a known variable star
00:46:11.97 +50:44:47.5 -- not a known variable star
00:46:14.54 +50:13:40.4 -- not a known variable star
00:46:15.15 +49:37:46.0 -- not a known variable star
00:46:17.92 +49:55:56.4 -- not a known variable star
00:46:18.32 +50:52:22.2 -- not a known variable star
00:46:18.71 +50:55:13.5 -- a known variable star
00:46:23.97 +49:40:43.6 -- a known variable star
00:46:26.92 +51:18:33.0 -- not a known variable star
00:46:30.01 +51:10:00.8 -- not a known variable star
00:46:31.50 +51:13:43.9 -- not a known variable star
00:46:38.70 +50:41:13.3 -- not a known variable star
00:46:38.80 +50:30:06.2 -- not a known variable star
00:46:39.22 +51:36:36.2 -- not a known variable star
00:46:43.15 +49:55:58.5 -- not a known variable star
00:46:45.82 +50:14:20.7 -- not a known variable star
00:46:46.22 +49:46:26.9 -- not a known variable star
00:46:47.03 +51:14:07.0 -- not a known variable star
00:46:48.49 +58:10:11.1 -- not a known variable star
00:46:51.47 +50:27:44.6 -- not a known variable star
00:46:53.36 +50:47:03.4 -- not a known variable star
00:46:53.59 +49:51:36.0 -- not a known variable star
00:46:54.69 +50:39:25.0 -- not a known variable star
00:47:00.30 +58:07:18.8 -- a known variable star
00:47:01.14 +51:22:05.0 -- not a known variable star
00:47:01.70 +50:42:52.3 -- a known variable star
00:47:02.28 +50:32:18.5 -- not a known variable star
00:47:07.85 +50:10:53.4 -- not a known variable star
00:47:14.56 +50:21:14.0 -- not a known variable star
00:47:16.25 +50:51:07.5 -- not a known variable star
00:47:24.18 +50:34:15.5 -- not a known variable star
00:47:33.94 +51:22:13.1 -- a known variable star
00:47:34.39 +50:57:36.5 -- not a known variable star
00:47:37.20 +50:24:26.3 -- not a known variable star
00:47:38.64 +51:01:39.2 -- not a known variable star
00:47:41.64 +50:48:50.0 -- not a known variable star
00:47:41.69 +50:47:29.4 -- a known variable star
00:47:47.57 +50:59:21.3 -- not a known variable star
00:47:48.52 +50:46:25.5 -- not a known variable star
00:47:48.94 +51:15:14.7 -- not a known variable star
00:47:50.76 +51:30:48.7 -- not a known variable star
00:47:53.87 +51:24:28.5 -- not a known variable star
00:47:56.81 +51:05:58.0 -- a known variable star
00:48:01.29 +53:47:45.1 -- not a known variable star
00:48:02.30 +50:47:44.6 -- not a known variable star
00:48:02.49 +51:33:32.7 -- not a known variable star
00:48:11.86 +50:59:22.9 -- not a known variable star
00:48:12.06 +50:51:51.2 -- not a known variable star
00:48:19.07 +50:56:33.0 -- not a known variable star
00:48:23.17 +54:48:53.2 -- not a known variable star
00:48:36.44 +51:29:37.3 -- not a known variable star
00:48:47.12 +51:11:36.0 -- not a known variable star
00:48:48.54 +51:15:20.3 -- a known variable star
00:48:55.16 +53:00:35.8 -- not a known variable star
00:49:00.11 +51:55:18.7 -- not a known variable star
00:49:38.43 +51:51:57.0 -- not a known variable star
00:49:49.28 +51:59:45.6 -- not a known variable star
00:50:42.09 +57:57:35.7 -- not a known variable star
00:53:07.27 +54:59:06.0 -- a known variable star
00:53:12.38 +54:48:07.2 -- not a known variable star
00:54:51.88 +56:45:46.4 -- not a known variable star
00:55:31.18 +56:33:11.6 -- not a known variable star
00:56:43.95 +57:23:36.4 -- not a known variable star
00:56:52.48 +57:23:42.3 -- not a known variable star
00:57:24.04 +57:00:13.7 -- not a known variable star
23:08:22.62 +55:49:47.2 -- not a known variable star
23:08:57.49 +53:23:18.7 -- not a known variable star
23:10:51.78 +54:50:07.5 -- a known variable star
23:11:31.33 +56:01:29.3 -- a known variable star
23:16:02.64 +53:58:02.4 -- a known variable star
23:16:48.80 +55:26:59.8 -- not a known variable star
23:17:32.89 +51:47:07.0 -- not a known variable star
23:20:45.39 +53:43:33.9 -- not a known variable star
23:23:16.71 +52:26:44.9 -- not a known variable star
23:24:32.34 +57:07:12.4 -- not a known variable star
23:25:05.02 +55:05:34.3 -- not a known variable star
23:25:30.77 +57:09:53.7 -- not a known variable star
23:28:31.85 +53:36:18.8 -- not a known variable star
23:29:14.19 +53:24:27.1 -- a known variable star
23:31:09.43 +54:16:19.7 -- not a known variable star
23:31:45.01 +54:09:37.0 -- not a known variable star
23:32:20.38 +54:04:39.5 -- not a known variable star
23:33:31.05 +52:42:15.6 -- not a known variable star
23:33:41.18 +49:58:08.9 -- not a known variable star
23:35:49.76 +51:16:44.8 -- not a known variable star
23:36:42.81 +52:12:23.4 -- a known variable star
23:38:10.97 +52:49:00.8 -- a known variable star
23:38:36.59 +57:11:43.8 -- not a known variable star
23:42:21.26 +57:04:54.2 -- not a known variable star
23:49:50.08 +53:26:58.0 -- a known variable star
23:57:50.00 +56:34:46.4 -- not a known variable star
Found 354 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
419 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 419 (excluding asteroids and hot pixels, 354 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)2461231.69821250 -observatory V36
07:32:40.19 +17:08:25.7 Mercury (5.0mag)
10:11:00.10 +12:45:00.9 Venus (-4.1mag)
04:23:43.02 +21:24:02.6 Mars (1.3mag)
08:16:32.20 +20:11:55.3 Jupiter (-1.8mag)
00:55:49.88 +03:20:25.2 Saturn (0.7mag)
04:07:12.25 +20:44:58.6 Uranus (5.8mag)
00:17:01.52 +00:20:42.0 Neptune (7.8mag)
20:30:55.79 -23:17:56.5 Pluto (14.4mag)
03:00:49.13 +21:28:26.1 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 361 Jul 9 23:58 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.69821250:
-rw-r--r-- 1 apache apache 0 Jul 9 23:58 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.69821250:
-rw-r--r-- 1 apache apache 0 Jul 9 23:58 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.69821250 -observatory V36
02:36:02.96 +14:24:35.0 17.9mag P/1996 R2 (Lagerkvist)
18:18:03.71 -34:21:29.6 13.7mag P/2010 H2 (Vales)
06:25:31.17 -68:08:14.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:45.11 +32:26:39.7 17.6mag C/2017 K2 (PANSTARRS)
17:03:09.66 +16:02:57.4 18.0mag C/2021 G2 (ATLAS)
01:46:54.36 +07:54:32.3 15.4mag P/2021 N1 (ZTF)
22:59:37.36 +32:17:07.8 17.3mag C/2022 E2 (ATLAS)
06:12:13.35 +26:55:39.3 16.7mag C/2022 N2 (PANSTARRS)
09:55:22.86 +29:47:16.2 16.8mag C/2022 QE78 (ATLAS)
09:09:38.14 +04:59:46.3 17.8mag C/2022 R6 (PANSTARRS)
18:07:18.79 +21:17:58.5 17.9mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:36.25 -11:23:03.8 17.7mag P/2023 B1 (PANSTARRS)
21:49:25.19 +67:37:18.2 17.8mag C/2023 H5 (Lemmon)
16:31:11.61 -10:03:43.8 13.9mag C/2023 R1 (PANSTARRS)
08:00:22.96 +65:42:01.3 17.9mag C/2024 A1 (ATLAS)
07:32:36.62 +29:59:43.7 14.6mag C/2024 E1 (Wierzchos)
15:16:24.13 +15:19:27.1 17.5mag C/2024 G6 (ATLAS)
19:41:30.38 +39:21:44.9 13.8mag C/2024 J3 (ATLAS)
21:47:44.43 +45:58:47.0 17.8mag C/2024 R4 (PANSTARRS)
04:49:29.55 -13:48:10.7 15.7mag C/2024 T5 (ATLAS)
06:34:26.60 +29:05:43.6 18.0mag C/2025 J1 (Borisov)
07:14:13.62 -12:52:34.7 16.4mag C/2025 R3 (PANSTARRS)
09:55:54.80 +22:26:36.4 17.6mag C/2025 V2 (Rankin)
12:44:34.01 +03:56:39.4 17.1mag C/2025 Y1 (ATLAS)
16:52:24.25 +79:07:00.9 17.4mag C/2026 A2 (Bok)
02:46:06.48 +45:13:57.8 16.7mag C/2026 B2 (Sun-Gao)
11:25:24.82 +04:30:59.0 16.9mag A/2026 E1
21:18:48.38 -15:01:19.0 7.3mag 10P/Tempel
11:13:22.99 -01:52:50.6 16.1mag 29P/Schwassmann-Wachmann
03:59:56.87 +29:32:10.2 17.8mag 47P/Ashbrook-Jackson
10:07:45.16 +14:03:37.8 17.0mag 63P/Wild
00:48:17.62 -05:05:42.3 15.6mag 65P/Gunn
08:26:28.10 +34:13:33.8 17.9mag 76P/West-Kohoutek-Ikemura
04:27:01.36 +20:10:13.2 13.7mag 78P/Gehrels
02:22:04.83 +10:35:15.8 16.2mag 88P/Howell
06:35:04.01 +30:32:36.3 15.7mag 93P/Lovas
04:20:29.84 +31:06:56.7 16.9mag 114P/Wiseman-Skiff
08:08:18.90 +30:43:13.6 15.3mag 123P/West-Hartley
10:47:50.56 +01:14:59.0 16.8mag 124P/Mrkos
04:51:28.69 +20:48:29.9 16.2mag 128P/Shoemaker-Holt
05:35:57.71 +19:42:53.9 17.8mag 131P/Mueller
00:01:30.14 +02:55:44.4 17.9mag 139P/Vaisala-Oterma
07:12:59.07 +17:03:13.4 15.5mag 141P-D/Machholz
03:16:46.79 -21:07:07.6 15.5mag 161P/Hartley-IRAS
05:32:30.30 +33:54:52.2 15.3mag 162P/SidingSpring
19:04:52.22 +14:59:22.8 14.7mag 169P/NEAT
01:40:39.52 +07:34:50.6 17.7mag 220P/McNaught
16:35:59.78 -08:22:46.7 17.0mag 235P/LINEAR
08:44:57.45 +33:18:49.1 17.9mag 240P/NEAT
20:42:14.85 -49:32:07.3 17.8mag 259P/Garradd
01:58:52.43 +12:01:20.4 15.7mag 260P/McNaught
05:36:45.37 +36:49:48.0 17.4mag 295P/LINEAR
15:06:37.43 +06:04:13.8 17.6mag 391P/Kowalski
08:34:27.86 +19:40:58.9 17.9mag 450P/LONEOS
07:51:31.32 +39:13:44.4 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 9 23:58 comets.txt
############################################################
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
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 9 23:58 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
20:32:17.644 -16:37:51.49 AT 2026sqa 2026-07-07.33 21.6569
20:38:02.144 -16:39:15.94 AT 2026spz 2026-07-07.33 22.7762
20:36:24.191 -15:13:43.37 AT 2026spy 2026-07-07.33 22.1739
20:41:10.988 -25:49:45.49 AT 2026spx 2026-07-07.33 22.8645
21:17:15.336 -23:31:53.39 AT 2026spw 2026-07-07.32 21.9459
20:27:45.431 -19:59:58.81 AT 2026spv 2026-07-07.33 21.6485
21:55:34.604 -14:11:57.66 AT 2026spu 2026-07-07.39 23.0585
21:10:34.181 -22:59:24.76 AT 2026spt 2026-07-07.32 22.3526
21:05:55.405 -19:04:02.26 AT 2026sps 2026-07-07.32 21.4424
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
20:31:34.503 -19:06:25.71 AT 2026spq 2026-07-07.33 22.7105
20:54:43.024 -26:43:41.99 AT 2026spp 2026-07-07.32 22.8017
21:07:49.748 -22:55:35.56 AT 2026spo 2026-07-07.32 22.494
20:57:55.962 -26:08:04.97 AT 2026spn 2026-07-07.32 22.7486
20:52:11.463 -28:17:09.07 AT 2026spm 2026-07-07.32 21.7705
21:10:07.376 -16:54:40.86 AT 2026spl 2026-07-07.32 22.4035
20:40:48.822 -16:22:21.53 AT 2026spk 2026-07-07.33 22.5822
12:31:52.422 +08:11:55.00 AT 2026spj 2026-07-07.05 22.147
21:57:34.362 -10:26:18.14 AT 2026spi 2026-07-07.39 22.5638
20:47:28.637 -25:46:50.92 AT 2026sph 2026-07-07.33 22.7363
-rw-r--r-- 1 apache apache 30K Jul 9 23:58 tns_transients_list.txt
